Quantum math: the rules – all of them! :-)

Pre-script (dated 26 June 2020): Our ideas have evolved into a full-blown realistic (or classical) interpretation of all things quantum-mechanical. In addition, I note the dark force has amused himself by removing some material. So no use to read this. Read my recent papers instead. šŸ™‚

Original post:

In my previous post, I made no compromise, and used allĀ of the rules one needs to calculate quantum-mechanical stuff:

Capture

However, I didn’t explain them. These rules look simple enough, but let’s analyze them now. They’re simple and not at the same time, indeed.

[I] The first equation uses the KroneckerĀ delta, which sounds fancy but it’s just a simple shorthand:Ā Ī“ijĀ =Ā Ī“jiĀ is equal to 1 if i = j, and zero if i ≠ j, withĀ iĀ andĀ jĀ representingĀ baseĀ states.Ā Equation (I) basically says that base states are all different.Ā For example, the angular momentum in the x-direction of a spin-1/2 particle – think of an electron or a proton – isĀ eitherĀ +ħ/2 orĀ āˆ’Ä§/2, not something in-between, or someĀ mixture. So 〈 +xĀ |Ā +x 〉 = 〈 āˆ’xĀ |Ā āˆ’x 〉 = 1 and 〈 +xĀ |Ā āˆ’x 〉 = 〈 āˆ’xĀ | +x 〉 = 0.

We’re talking base states here, of course. Base states are like a coordinate system: we settle on an x-, y- and z-axis, and a unit, and any point is defined in terms of an x-, y– and z-number. It’s the same here, except we’re talking ‘points’ in four-dimensional spacetime. To be precise, we’re talking constructs evolving in spacetime. To be even more precise, we’re talking amplitudesĀ with a temporal as well as a spatial frequency, which we’ll often represent as:

aĀ·eāˆ’iĀ·ĪøĀ =Ā eāˆ’iĀ·(ω·t āˆ’ kĀ āˆ™x)Ā =Ā aĀ·eāˆ’(i/ħ)Ā·(EĀ·t āˆ’ pāˆ™x)

The coefficient in front (a) is just a normalization constant, ensuring all probabilities add up to one. It may not be a constant, actually: perhaps it just ensure our amplitude stays within some kind of envelope, as illustrated below.

Photon wave

As for the ω = E/ħ and k =Ā p/ħ identities, these are the de Broglie equations for aĀ matter-wave, which the young ComteĀ jotted down as part of his 1924 PhD thesis. He was inspired by the fact that theĀ EĀ·t āˆ’ pāˆ™xĀ factor is an invariantĀ four-vector productĀ (EĀ·t āˆ’ pāˆ™x =Ā pμxμ) in relativity theory, and noted the striking similarity with the argument of any wave function in space and time (ω·t āˆ’ kĀ āˆ™x) and, hence, couldn’t resist equating both. Louis de Broglie was inspired, of course, by the solution to the blackbody radiation problem, which Max Planck and Einstein had convincingly solved by accepting that the ω = E/ħ equation holds for photons. As he wrote it:

“When I conceived the first basic ideas of wave mechanics in 1923–24, I was guided by the aim to perform a real physical synthesis, valid for all particles, of the coexistence of the wave and of the corpuscular aspects that Einstein had introduced for photons in his theory of light quanta in 1905.” (Louis de Broglie, quoted in Wikipedia)

Looking back, you’d of course want the phase of a wavefunction to be some invariant quantity, and the examples we gave our previous post illustrate how one would expect energy and momentum to impact its temporal and spatial frequency. But I am digressing. Let’s look at the second equation. However, before we move on, note thatĀ minusĀ sign in the exponent of our wavefunction:Ā aĀ·eāˆ’iĀ·Īø. The phase turns counter-clockwise. That’s just the way it is. I’ll come back to this.

[II] The φ and χ symbols do notĀ necessarily represent base states. In fact, Feynman illustrates this law using a variety of examples including both polarized as well asĀ unpolarizedĀ beams, or ‘filtered’ as well as ‘unfiltered’ states, as he calls it in the context of the Stern-Gerlach apparatuses he uses to explain what’s going on. Let me summarize his argument here.

I discussed the Stern-Gerlach experiment in myĀ post on spin and angular momentum, but the Wikipedia article on it is very good too. The principle is illustrated below: a inhomogeneous magnetic field – note the direction of the gradient āˆ‡B = (āˆ‚B/āˆ‚x, āˆ‚B/āˆ‚y, āˆ‚B/āˆ‚z) – will split a beam of spin-one particles into three beams. [Matter-particles with spin one are rather rare (Lithium-6 is an example),Ā but three states (rather than two only, as we’d have when analyzing spin-1/2 particles, such as electrons or protons) allow for more playĀ in the analysis. šŸ™‚ In any case, the analysis is easily generalized.]

stern-gerlach simple

The splitting of the beam is based, of course, on the quantized angular momentum in the z-directionĀ (i.e. the direction of the gradient): its value is either ħ, 0, or āˆ’Ä§. We’ll denote theseĀ baseĀ states as +, 0 orĀ āˆ’, and we should note they are defined in regard to an apparatus with a specific orientation. If we call this apparatus S, then we can denote theseĀ base states as +S, 0S and āˆ’S respectively.

The interesting thing in Feynman’s analysis is the imagined modifiedĀ Stern-Gerlach apparatus, which – I am using Feynman‘s words here šŸ™‚Ā ā€“ Ā “puts Humpty Dumpty back together.” It looks a bit monstruous, but it’s easy enough to understand. Quoting Feynman once more: “It consists of a sequence of three high-gradient magnets. The first one (on the left) is just the usual Stern-Gerlach magnet and splits the incoming beam of spin-one particles into three separate beams. The second magnet has the same cross section as the first, but is twice as long and the polarity of its magnetic field is opposite the field in magnetĀ 1. The second magnet pushes in the opposite direction on the atomic magnets and bends their paths back toward the axis, as shown in the trajectories drawn in the lower part of the figure. The third magnet is just like the first, and brings the three beams back together again, so that leaves the exit hole along the axis.”

stern-gerlach modified

Now, we can use this apparatus as aĀ filterĀ by inserting blocking masks, as illustrated below.

filter

But let’s get back to the lesson. What about the second ‘Law’ of quantum math? Well… You need to be able to imagine all kinds of situations now. The rather simple set-up below is one of them: we’ve got two of these apparatuses in series now, S and T, with T tilted at the angle α with respect to the first.

tilted

I know: you’re getting impatient. What about it? Well… We’re finally ready now. Let’s suppose we’ve got three apparatuses in series, with the first and the last one having the very same orientation, and the one in the middle being tilted. We’ll denote them by S, T and S’ respectively. We’ll also use masks: we’ll block the 0 andĀ āˆ’ state in the S-filter, like in that illustration above. In addition, we’ll block the + andĀ āˆ’ state in the T apparatus and, finally, the 0 andĀ āˆ’ state in the S’ apparatus. Now try to imagine what happens: how many particles will get through?

[…]

Just try to think about it.Ā Make some drawing or something. Please!Ā Ā 

[…]

OK… The answer is shown below. Despite the filtering in S, the +S particles that come out do have an amplitude to go through the 0T-filter, and so the number of atoms that come out will be some fraction (α) of the number of atoms (N) that came out of the +S-filter. Likewise, some other fraction (β) will make it through the +S’-filter, so we end up with βαN particles.

ratio 2

Now, I am sure that, if you’d tried to guess the answer yourself, you’d have saidĀ zeroĀ rather than βαN but, thinking about it, it makes sense: it’s not because we’ve got some angular momentum in one direction that we have none in the other. When everything is said and done, we’re talking componentsĀ of theĀ total angular momentum here, don’t we? Well… Yes and no. Let’s remove the masks from T. What do we get?

[…]

Come on: what’s your guess? N?

[…] You’re right. It’s N. Perfect. It’s what’s shown below.

ratio 3

Now,Ā thatĀ should boost your confidence. Let’s try the next scenario. We block the 0 andĀ āˆ’ state in the S-filter once again, and theĀ + andĀ āˆ’ state in the T apparatus, so the first two apparatuses are the same as in our first example. But let’s change the S’ apparatus: let’s close the + andĀ āˆ’ state there now. Now try to imagine what happens: how many particles will get through?

[…]

Come on! You think it’s a trap, isn’t it? It’s not. It’s perfectly similar: we’ve got some other fraction here, which we’ll write as γαN, as shown below.

ratio 1Next scenario: S has the 0 andĀ āˆ’ gate closed once more, and T is fully open, so it has no masks. But, this time, we set S’ so it filters the 0-state with respect to it. What do we get? Come on!Ā Think! Please!

[…]

The answer is zero, as shown below.

ratio 4

Does that make sense to you? Yes? Great! Because many think it’s weird: they think the T apparatus must ‘re-orient’ the angular momentum of the particles. It doesn’t: if the filter is wide open, then “no information is lost”, as Feynman puts it. Still… Have a look at it. It looks like we’re opening ‘more channels’ in the last example: the S and S’ filter are the same, indeed, and T is fully open, while it selected for 0-state particles before. ButĀ noĀ particles come through now, while with the 0-channel, we had γαN.

Hmm… It actuallyĀ isĀ kinda weird, won’t you agree?Ā Sorry I had to talk about this, but it will make you appreciate that secondĀ ‘Law’ now: we can always insert a ‘wide-open’ filter and, hence, split the beams into a completeĀ set of base statesĀ āˆ’ with respect to the filter, that isĀ āˆ’Ā and bring them back together provided our filter does not produce any unequal disturbances on the three beams. In short, the passage through the wide-open filter shouldĀ notĀ result in a change of the amplitudes. Again, as Feynman puts it: the wide-open filter should really put Humpty-Dumpty back together again. If it does, we can effectively apply our ‘Law’:

second law

For an example, I’ll refer you to my previous post. This brings me to the third and final ‘Law’.

[III]Ā The amplitude to go from state φ to state χ is the complex conjugateĀ of the amplitude to to go from state χ to state φ:

〈 χ |Ā Ļ†Ā āŒŖ = 〈 φ | Ļ‡Ā āŒŖ*

This is probably the weirdest ‘Law’ of all, even if I should say, straight from the start, we can actually derive it from the second ‘Law’, and the fact that all probabilities have to add up to one. Indeed, a probability is theĀ absoluteĀ square of an amplitude and, as we know, theĀ absoluteĀ square of a complex number is also equal to the product of itself and its complex conjugate:

|z|2Ā =Ā |z|Ā·|z| = zĀ·z*

[You should go through the trouble of reviewing the difference between the square and the absoluteĀ square of a complex number. Just write z as a + ib and calculate (a + ib)2Ā = a2Ā + 2abiĀ + b2 , as opposed to |z|2Ā = a2Ā + b2. Also check what it means when writing z as rĀ·eiĪøĀ = rĀ·(cosĪø + iĀ·sinĪø).]

Let’s applying the probability rule to a two-filter set-up, i.e. the situation with the S and the tilted T filter which we described above, and let’s assume we’ve got a pure beam of +S particles entering the wide-open T filter, so our particles can come out in either of the three base states with respect to T. We can then write:

〈 +TĀ |Ā +S 〉2Ā + 〈 0T |Ā +S 〉2Ā + 〈 āˆ’T | +S 〉2Ā = 1

⇔ 〈 +TĀ |Ā +S 〉〈 +TĀ |Ā +S 〉* + 〈 0T |Ā +S 〉〈 0T |Ā +S 〉* + 〈 āˆ’T | +S 〉〈 āˆ’T | +S 〉* = 1

Of course, we’ve got two other such equations if we start with a 0S or aĀ āˆ’S state. Now, we take the 〈 χ |Ā Ļ†Ā āŒŖ =Ā āˆ‘ 〈 χ | i 〉〈 i |Ā Ļ†Ā āŒŖ ‘Law’, and substitute χ and φ for +S, andĀ allĀ iĀ states for the base states with regard to T. We get:

〈 +S | +S 〉 = 1 = 〈 +S |Ā +T 〉〈 +TĀ |Ā +S 〉 + 〈 +S | 0T 〉〈 0T |Ā +S 〉 + 〈 +S | –T 〉〈 āˆ’T | +S 〉

These equations are consistent only if:

〈 +S | +T 〉 = 〈 +T | +S 〉*,

〈 +S | 0T 〉 = 〈 0T | +S 〉*,

〈 +S |Ā āˆ’T 〉 = 〈 āˆ’T |Ā +S 〉*,

which is what we wanted to prove. One can then generalize to any state φ and χ. However, provingĀ the result is one thing.Ā Understanding it is something else. One can write down a number of strange consequences, which all point to Feynman‘s rather enigmatic comment on this ‘Law’:Ā “If this Law were not true, probability would not be ‘conserved’, and particles would get ‘lost’.” So what doesĀ thatĀ mean?Ā Well… You may want to think about the following, perhaps. It’s obvious that we can write:

|〈 φ | Ļ‡Ā āŒŖ|2Ā = 〈 φ | Ļ‡Ā āŒŖāŒ© φ | Ļ‡Ā āŒŖ* = 〈 χ | φ 〉*〈 χ | φ 〉 =Ā |〈 χ | φ 〉|2

This says that the probability to go from the φ-state to the χ-state Ā isĀ the sameĀ as the probability to go from the χ-state to the φ-state.

Now, when we’re talking base states, that’s rather obvious, because the probabilities involved are either 0 or 1. However, if we substitute for +S and āˆ’T, or some more complicated states, then it’s a different thing. My guts instinct tells me this third ‘Law’ – which, as mentioned, can be derivedĀ from the other ‘Laws’ – reflectsĀ the principle ofĀ reversibilityĀ in spacetime, which you may also interpret as aĀ causalityĀ principle, in the sense that, in theory at least (i.e. not thinking about entropy and/or statistical mechanics), we can reverse what’s happening: we can go back in spacetime.

In this regard, we should alsoĀ remember that the complex conjugate of a complex number in polar form, i.e. a complex number written asĀ rĀ·eiĪø, is equal toĀ rĀ·eāˆ’iĪø, so the argument in the exponent gets aĀ minusĀ sign. Think about what this means for ourĀ aĀ·eāˆ’iĀ·ĪøĀ =Ā eāˆ’iĀ·(ω·t āˆ’ kĀ āˆ™x)Ā =Ā aĀ·eāˆ’(i/ħ)Ā·(EĀ·t āˆ’ pāˆ™x)Ā function. Taking the complex conjugate of this function amounts toĀ reversing the direction of t and x which, once again, evokes that idea of going back in spacetime.

I feel there’s some more fundamental principle here at work, on which I’ll try to reflect a bit more. Perhaps we can also do something with that relationship between the multiplicative inverse of a complex number and its complex conjugate, i.e.Ā zāˆ’1Ā = z*/|z|2. I’ll check it out. As for now, however, I’ll leave you to do that, and please let me know if you’ve got any inspirational ideas on this. šŸ™‚

So… Well… Goodbye as for now. I’ll probably talk about theĀ HamiltonianĀ in my next post. I think we really did a good job in laying the groundwork for the really hardcore stuff, so let’s go for that now. šŸ™‚

Post Scriptum: On the Uncertainty Principle and other rules

After writing all of the above, I realized I should add some remarks to make this post somewhat more readable. First thing: not all of the rules are there—obviously! Most notably, I didn’t say anything about the rules for adding or multiplying amplitudes, but that’s because I wrote extensively about that already, and so I assume you’re familiar with that. [If not, see my page on the essentials.]

Second, I didn’t talk about the Uncertainty Principle. That’s because I didn’t have to. In fact, we don’t need it here. In general, all popular accounts of quantum mechanics have an excessive focus on the position and momentum of a particle, while the approach in this and my previous post is quite different. Of course, it’s Feynman’s approach to QM really. Not ‘mine’. šŸ™‚ All of the examples and all of the theory he presents in his introductory chapters in the Third Volume of Lectures, i.e. the volume on QM, are related to things like:

  • What is the amplitude for a particle to go from spin state +S to spin state āˆ’T?
  • What is the amplitude for a particle to be scattered, by a crystal, or from some collision with another particle, in the Īø direction?
  • What is the amplitude for two identical particles to be scattered in the same direction?
  • What is the amplitude for an atom to absorb or emit a photon? [See, for example, Feynman’s approach to the blackbody radiation problem.]
  • What is the amplitude to go from one place to another?

In short, you read Feynman, and it’s only at theĀ veryĀ end of hisĀ exposĆ©, that he starts talking about the things popular books start with, such as the amplitude of a particle to be at point (x, t) in spacetime, or the Schrƶdinger equation, which describes the orbital of an electron in an atom. That’s where the Uncertainty Principle comes in and, hence, one can really avoid it for quite a while. In fact, oneĀ shouldĀ avoid it for quite a while, because it’s now become clear to me that simply presenting the Uncertainty Principle doesn’t help all that much to trulyĀ understandĀ quantum mechanics.

Truly understanding quantum mechanics involves understanding all of these weird rules above. To some extent, that involves dissociatingĀ the idea of the wavefunction with our conventional ideas of time and position. From the questions above, it should be obvious that ‘the’ wavefunction does actuallyĀ notĀ exist: we’ve got a wavefunction for anything we can and possibly want to measure. That brings us to the question of the base states: what areĀ they?

Feynman addresses this question in a rather verbose section of his Lectures titled:Ā What are the base states of the world?Ā I won’t copy it here, but I strongly recommend you have a look at it. šŸ™‚

I’ll end here with a final equation that we’ll need frequently: the amplitude for a particle to go from one place (r1) to another (r2). It’s referred to as aĀ propagatorĀ function, for obvious reasons—one of them being that physicists like fancy terminology!—and it looks like this:

propagator

The shape of theĀ e(i/ħ)Ā·(pāˆ™r12)Ā function is now familiar to you. Note theĀ r12Ā in the argument, i.e. the vectorĀ pointing fromĀ r1Ā to r2. The pāˆ™r12Ā dot product equals |p|āˆ™|r12|Ā·cosĪø = pāˆ™r12Ā·cosĪø, with Īø the angle between p and r12. If the angle is the same, then cosĪø is equal to 1. If the angle is Ļ€/2, then it’s 0, and the function reduces to 1/r12. So the angle Īø, through the cosĪø factor, sort of scalesĀ the spatial frequency. Let me try to give you some idea of how this looks like by assuming the angle between p and r12Ā is the same, so we’re looking at the space in the direction of the momentum only andĀ |p|āˆ™|r12|Ā·cosĪø = pāˆ™r12. Now, we can look at the p/ħ factor as a scalingĀ factor, and measure theĀ distance xĀ in units defined by that scale, so we write: x = pāˆ™r12/ħ.Ā The function then reduces to (ħ/p)Ā·eiāˆ™x/xĀ =Ā (ħ/p)Ā·cos(x)/xĀ + iĀ·(ħ/p)Ā·sin(x)/x, and we just need to square this to get the probability. All of the graphs are drawn hereunder: I’ll let you analyze them. [Note that the graphs do not include the ħ/p factor, which you may look at as yet another scaling factor.] You’ll see – I hope! – that it all makes perfect sense: the probability quickly drops off with distance, both in the positive as well as in the negative x-direction, while it’s going to infinity when veryĀ near.Ā [Note that the absolute square, usingĀ cos(x)/xĀ andĀ sin(x)/xĀ yields the same graph as squaring 1/x—obviously!]

graph

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Taking the magic out of God’s number: some additional reflections

Note: I have published a paper that is very coherent and fully explains this so-called God-given number. There is nothing magical about it. It is just a scaling constant. Check it out: The Meaning of the Fine-Structure Constant. No ambiguity. No hocus-pocus.

Jean Louis Van Belle, 23 December 2018

Original post:

In my previous post, I explained why the fine-structure constant α isĀ notĀ a ‘magical’ number, even ifĀ it relates all fundamental properties of the electron: its mass, its energy, its charge, its radius, its photonĀ scattering cross-sectionĀ (i.e. the Bohr radius, or the size of the atom really) and, finally, the couplingĀ constant for photon-electron interactions.Ā The key to such understanding of α was the model of an electron as a tiny ball of charge. As such, we have two energy formulas for it. One is the energy that’s needed to assemble the charge from infinitely dispersed infinitesimal charges, which we denoted as Uelec. The other formula is the energy of the fieldĀ of the tiny ball of charge, which we denoted as Eelec.

The formula for EelecĀ is calculated using the formula for the field momentum of a moving charge and, using the m = E/c2Ā mas-energy equivalence relationship, is equivalentĀ to the electromagnetic mass. We went through the derivation in our previous post, so let me just jot down the result:

emm - 2

The second formula depends on what ball of charge we’re thinking of, because the formulas for a charged sphere and aĀ sphericalĀ shellĀ of charge are different: both have the same structureĀ as the relationship above (so the energy is also proportional to the square of the electron charge andĀ inverselyĀ proportional to the radius a), but the constant of proportionality is different. For a sphere of charge, we write:

Ā f sphre

For a spherical shellĀ of charge we write:

shell

To compare the formulas, you need to note that the square of the electron chargeĀ eĀ in the formula for the field energy isĀ equal to e2Ā = qe2/4πε0Ā = keĀ·qe2. So we multiplyĀ the square of the actualĀ electron charge by the Coulomb constant keĀ = 1/4πε0. As you can see, the three formulas have exactlyĀ the same form then. It’s just the proportionality constant that’s different: it’s 2/3, 3/5 and 1/2 respectively.Ā It’s interesting to quickly reflect on the dimensions here: [ke] ā‰ˆ 9Ɨ109 NĀ·m2/C2, so e2Ā is expressed in NĀ·m2. That makes the units come out alright, as we divide by a (so that’s in meter) and so we get the energy inĀ jouleĀ (which is newtonĀ·meter). In fact, now that we’re here, let’s quickly calculate the value of e2: it’s that keĀ·qe2Ā product, so it’s equal to 2.3Ɨ10āˆ’28Ā NĀ·m2. We can quickly check this value because we know that the classical electron radius is equal to:

classical electron radius

So we divide 2.3Ɨ10āˆ’28Ā NĀ·m2Ā by mec2Ā ā‰ˆ 8.2Ɨ10āˆ’14 J, so we get r0Ā ā‰ˆ 2.82Ɨ10āˆ’15Ā m. So we’re spot on! Why did I do this check? Not really to check what I wrote. It’s more to show what’s going on.Ā We’ve got yet another formula relating the energy and the radius of an electron here, so now we have three. In fact we have more because the formula for UelecĀ depends on the finer details of our model for the electron (sphere versus shell, uniform versus non-uniform distribution):

  1. EelecĀ = (2/3)Ā·(e2/a): This is the formula for the energy of the field, so we may all it isĀ externalĀ energy.
  2. UelecĀ = (3/5)Ā·(e2/a), or UelecĀ = (1/2)Ā·(e2/a): This is the energy needed to assembleĀ our electron, so we might, perhaps, call it itsĀ internalĀ energy. The first formula assumes our electron is a uniformly chargedĀ sphere. The second assumes all charges sit on the surface of the sphere. If we drop the assumption of the charge having to be uniformly distributed, we’ll find yet another formula.
  3. mec2Ā =Ā e2/r0: This is the energy associated with the so-called classical electron radiusĀ (r0) and the electron’s rest mass (me).

In our previous posts, we assumed the last equation was the right one. Why? Because it’s the one that’s been verified experimentally. The discrepancies between the various proportionality coefficients – i.e. the difference between 2/3 and 1, basically – are to be explained because of theĀ binding forces within the electron, without which the electron would just ‘explode’, as the French physicist and polymath Henri PoincarĆ© famously put it.Ā Indeed, if the electron is a little ball of negative charge, the repulsive forces between its parts should rip it apart. So we will not say anything more about this. You can have fun yourself byĀ googlingĀ all the various theories that try to model these binding forces. [I may do the same some day, but now I’ve got other priorities: I want to move to Feynman’s third volume ofĀ Lectures, which is devoted to quantum physicsĀ only, so I look very much forward to that.]

In this post, I just wanted to reflect once more on what constants are reallyĀ fundamentalĀ and what constants are somewhat less fundamental. From all what I wrote in my previous post, I said there were three:

  1. The fine-structure constant α, which is a dimensionless number.
  2. Planck’s constant h, whose dimension is jouleĀ·second, so that’s the dimension ofĀ action.
  3. The speed of light c, whose dimension is that of a velocity.

The three are related through the following expression:

alpha re-expressed

This is an interesting expression. Let’s first check its dimension. We already explained thatĀ e2Ā is expressed inĀ NĀ·m2. That’s rather strange, because it means the dimension of e itself is N1/2Ā·m: what’s the square root of a force of oneĀ newton? In fact, to interpret the formula above, it’s probably better to re-writeĀ e2Ā asĀ e2Ā = qe2/4πε0Ā = keĀ·qe2. That shows you how the electron charge and Coulomb’s constant are related. Of course, they are part and parcel of one and the same force law:Ā Coulomb’s law. We don’t need anything else, except for relativity theory, because we need to explain theĀ magnetic forceĀ as well—andĀ thatĀ we can do because magnetism is just a relativistic effect. Think of the field momentum indeed: the magnetic field comes into play only when we start to move our electron. The relativity effect is captured by cĀ  in that formula for α above. As for ħ, ħ = h/2Ļ€ comes with the E = hĀ·fĀ equation, which links us to the electron’s Compton wavelengthĀ Ī» through theĀ de BroglieĀ relationĀ Ī» = h/p.

The point is: we should probably not look at α as a ‘fundamental physical constant’. It’s e2Ā that’s the third fundamental constant, besides h and c. Indeed, it’s fromĀ e2Ā that all the rest follows: the electron’s internal energy, its external energy, and its radius, and then all the rest by combining stuff with other stuff.

Now, we took the magic out of α by doing what we did in the previous posts, and that’s to combine stuff with other stuff, and so now you may think I am putting the magic back in with that formula for α, which seems to define α in terms of the three mentioned ‘fundamental’ constants. That’s not the case: this relation comes out of all of the other relationships we found, and so it’s nothing new really. It’s actually notĀ a definition of α: it just does what it does, and that’s toĀ relate α to the ‘fundamental’ physical constants behind.

So… No new magic. In fact, I want to close this post by taking away even more of the magic. If you read my previous post, I said that α was ‘God’s cut-off factor’ šŸ™‚ ensuring our energy functions do not blow up, but I also said it was impossible to sayĀ whyĀ he choseĀ 0.00729735256Ā as the cut-off factor. The question is actually easily answered by thinking about thoseĀ twoĀ formulas we had for the internal and external energy respectively. Let’s re-write them in natural units and, temporarily, two different subscripts for α, so we write:

  1. Eelec = αe/r0: This is the formula for the energy of the field.
  2. Uelec = αu/r0: This is the energy needed to assemble our electron.

Both energies are determined by the above-mentioned laws, i.e. Coulomb’s Law and the theory of relativity, so α has got nothing to do what that. However, both energies have to be the same, and so αeĀ has to be equal to αu. In that sense, α is, quite simply, aĀ proportionality constantĀ that achieves that equality. NowĀ thatĀ explains why we canĀ derive α from the three other constants which, as mentioned above, are probablyĀ moreĀ fundamental. In fact, we’ve got only three degrees of freedom here, so if we chose c,Ā h andĀ eĀ as ‘fundamental’, then α isn’t any more.

The underlying deep question behind it all isĀ whyĀ those two energies should be equal.Ā Why would our electron have some internal energy if it’s elementary? The answer to that question is: because it has some non-zero radius, and it has some non-zero radius because we don’t want our formula for the field energy (or the field momentum) to blow up. Now, if it has some radius, then itĀ hasĀ to have some internal energy.

You’ll say: that makes sense, but it doesn’t answer the question. Why would it haveĀ internal energy, with or without a zero radius? If an electron is an elementaryĀ particle, then it’s reallyĀ elementary, isn’t? And so then we shouldn’t try to ‘assemble’ it from an infinite number of infinitesimally small charges. You’re right, and here we can also note that the fact that the electron doesn’t blow up is firm evidence it’s veryĀ elementary indeed.

I should also note that Feynman actually doesn’t talk about the energy that’s needed to assemble a charge: he gets his UelecĀ = (1/2)Ā·(e2/a) by calculating the externalĀ field energy for a spherical shell of charge, and he sticks to it—presumably because it’s the same field for a uniform or non-uniformĀ sphere of charge. He only notes there has to be some radius because, if not, the formula he uses blows up, indeed. So – who knows? – perhaps he doesn’t quite believe that formula for theĀ internalĀ energy is relevant either.

So perhaps there is no internal energy indeed. Perhaps there’s just the energy of the field. So… Well… I can’t say much about this… Except… Well…Ā Perhaps just one more thing. Let me note somethingĀ that, I hope, you noticed as well: theĀ keĀ·qe2 is the numerator in Coulomb’s Law itself. You also know that energy equals force times distance. So if we divide both sides by r0, we get Coulomb’s Law itself FelecĀ = keĀ·qe2/r02. The only thing is: what’s the distance? It’s one charge only, and there is no distance between one charge, is there? Well… Yes and no. I have been thinking that the requirement of the internal and external energies being equal resembles the statement that the forces between two charges are equal and opposite. That ties in with the idea of the internal energy itself: remember we were basically talking forces between infinitesimally small elements of charge within the electron itself? So r0Ā is, perhaps, some averageĀ distance or so. There must beĀ someĀ way of thinking of it like that. But… Well… Which oneĀ exactly?

This kind of reflection may not make sense. Who knows? I obviously need to think all of this through and so this post is, indeed, just a bunch of reflections for which I will have more time later—hopefully. šŸ™‚ Perhaps we’re all just pushing the matter too far. Perhaps we should just accept that the external energy has that 2/3 factor but that the actual energy of the electron should also include the equivalent energy of some binding force that holds the electron together. Well… In any case. That’s all I am going to do on this extremely complicated matter. It’s time to move indeed! So the point to take home here is probably just this:

  1. When calculating the radius of an electron using classical theory, we get in trouble: not only do we find different radii, but the radii that we find do not respect the E =Ā mec2Ā law. It’s only theĀ mec2Ā =Ā e2/r0Ā that’s relativistically correct.
  2. That suggests the electron also has some non-electric mass, which are referred to as ‘binding forces’ or ‘PoincarĆ© stresses’, but which remain to be explained convincingly.
  3. All of this shouldn’t surprise us: for all we know, the electron is something fuzzy. šŸ™‚

So my next posts will focus on the ‘essentials’ preparing for Feynman’s Volume on quantum mechanics. Those ‘essentials’ will still involve some classical stuff but, as you will see, even more contradictions, that – hopefully! – will then be solved in the quantum-mechanicalĀ picture of itĀ all. šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Taking the magic out of God’s number

Note: I have published a paper that is very coherent and fully explains this so-called God-given number. There is nothing magical about it. It is just a scaling constant. Check it out: The Meaning of the Fine-Structure Constant. No ambiguity. No hocus-pocus.

Jean Louis Van Belle, 23 December 2018

Original post:

I think the post scriptum to my previous post is interesting enough to separate it out as a piece of its own, so let me do that here. You’ll remember that we were trying to find some kind of a model for the electron, picturing it like a tiny little ball of charge, and then we just applied the classical energy formulas to it to see what comes out of it. TheĀ key formula is the integral that gives us the energy that goes into assembling a charge. It was the following thing:

U 4

This is a double integral which we simplified in two stages, so we’re looking at an integral within an integral really, butĀ we can substitute the integral over the ρ(2)Ā·dV2Ā product by the formula we got for the potential, so we write that as Φ(1), and so the integral above becomes:

U 5Now, thisĀ integral integrates the ρ(1)·Φ(1)Ā·dV1Ā product over all of space, so that’s over all points in space, and so we just dropped the index and wrote the whole thing as the integral of ρ·Φ·dVĀ over all of space:

U 6

We thenĀ established that this integral was mathematically equivalent to the following equation:

U 7

So this integral is actually quite simple: it just integrates E•E = E2Ā over all of space. The illustration below shows E as a function of the distanceĀ rĀ for a sphere of radius R filledĀ uniformlyĀ with charge.

uniform density

So the field (E) goes asĀ rĀ for r ≤ R and as 1/r2Ā for r ≄ R. So, for r ≄ R, the integral will have (1/r2)2Ā = 1/r4Ā in it. Now, you know that the integral of some function is the surface under the graph of that function. Look at the 1/r4 function below: it blows up between 1 and 0. That’s where the problem is: there needs to be some kind of cut-off, because that integral will effectively blow up when the radius of our little sphere of charge gets ‘too small’.Ā So that makes it clear why it doesn’t make sense to use this formula to try to calculate the energy of a point charge. It just doesn’t make sense to do that.

graph

In fact, the need for a ‘cut-off factor’ so as to ensure our energy function doesn’t ‘blow up’ is not because of the exponent in theĀ 1/r4 expression: the need is also there for any 1/r relation, as illustrated below. AllĀ 1/rnĀ function have the sameĀ pivotĀ point, as you can see from the simple illustration below. So, yes, we cannot go all the way to zero from there when integrating: we have to stopĀ somewhere.

graph 2So what’s the ‘cut-off point’? What’s ‘too small’ a radius? Let’s look at the formula we got for our electron as a shellĀ of charge (so the assumption here is that the charge isĀ uniformly distributed on the surfaceĀ of a sphere with radius a):

energy electron

So we’ve got an even simpler formula here: it’s just a 1/rĀ relation (a is rĀ in this formula), not 1/r4. Why is that? Well… It’s just the way the math turns out: we’re integrating over volumes and so that involves an r3Ā factor and so it all simplifies to 1/r, and so that gives us this simple inverselyĀ proportional relationship between U and r, i.eĀ a, in this case. šŸ™‚Ā I copied the detail of Feynman’s calculation in my previous post, so you can double-check it. It’s quite wonderful, really. Look at it again: we have a very simpleĀ inverselyĀ proportional relationship between theĀ radiusĀ of our electron andĀ itsĀ energy as a sphere of charge. We could write it as:

Uelect  = α/a, with α = e2/2

Still… We need the cut-off point’. Also note that, as I pointed out, we don’t necessarily need to assume that the charge in our little ball of charge (i.e. our electron) sits on the surface only: if we’d assume it’s a uniformly charged sphere of charge, we’d just get another constant of proportionality: our 1/2 factor would become a 3/5 factor, so we’d write: UelectĀ Ā = (3/5)Ā·e2/a. But we’re not interested in finding the rightĀ model here. We know theĀ UelectĀ Ā = (3/5)Ā·e2/aĀ gives us a value forĀ aĀ that differs with a 2/5 factor as the classical electron radius. That’s not so bad and so let’s go along with it. šŸ™‚

We’re going to look at the simpleĀ structureĀ of this relation, and all of its implications. The simple equation above says that the energy of our electron is (a) proportional to the square of its charge and (b) inversely proportional to its radius. Now,Ā thatĀ is a very remarkable result. In fact,Ā we’ve seen something like this before, and we were astonished.Ā We saw it when we were discussing the wonderful properties of that magical number, theĀ fine-structure constant, which we also denoted by α. However, because we used α already, I’ll denote the fine-structure constant as αe here, so you don’t get confused. You’ll remember thatĀ the fine-structure constant is a God-like number indeed: it links allĀ of the fundamental properties of the electron, i.e. its charge, its radius, its distance to the nucleus (i.e. the Bohr radius), its velocity, its mass (and, hence, its energy), its de BroglieĀ wavelength. Whatever: all these physical constants are all related through the fine-structure constant.Ā 

In my various posts on this topic, I’ve repeatedly said that, but I never showed why it’s true, and so it was a very magical number indeed. I am going to take some of the magic out now. Not too much but… Well… You can judge for yourself how much of the magic remains after I am done here. šŸ™‚

So, at this stage of the argument, α can be anything, and αeĀ cannot, of course. It’s just that magical number out there, which relates everything to everything: it’s the God-given number we don’t understand,Ā or didn’t understand, I should say. Past tense. Indeed, we’re going to get some understanding here because we know that one of theĀ many expressions involving αe was the following one:

me = αe/re

This says that theĀ massĀ of the electron is equal to the ratio of the fine-structure constant and the electron radius. [Note that we express everything in natural units here, so that’sĀ Planck units. For the detail of the conversion, please see the relevant section on that in my one of my posts on this and other stuff.] In fact, the U =Ā (3/5)Ā·e2/aĀ andĀ meĀ = αe/reĀ relations looks exactlyĀ the same, because one of the other equations involving the fine-structure constant was: αeĀ =Ā eP2. So we’ve got the square of the charge here as well! Indeed, as I’ll explain in a moment, the difference between the two formulas is just a matter of units.

Now, mass is equivalent to energy, of course: it’s just a matter of units, so we can equate meĀ with EeĀ (this amounts to expressing the energy of the electron in aĀ kg unit—bit weird, but OK) and so we get:

Ee = αe/re

So there we have: the fine-structure constant αeĀ is Nature’s ‘cut-off’ factor, so to speak. Why? Only God knows. šŸ™‚ But it’s now (fairly) easy to see why all the relations involving αeĀ are what they are. As I mentioned already, we also know that αeĀ is the square of the electron charge expressed in Planck units, so we have:

 αe = eP2 and, therefore, Ee = eP2/re

Now, you can check for yourself: it’s just a matter of re-expressing everything in standard SI units, and relating eP2Ā to e2, and it should all work: you should get the EelectĀ Ā = (2/3)Ā·e2/aĀ expression. So… Well… At least this takes some of the magic out the fine-structure constant. It’s still a wonderful thing, but so you see that the fundamental relationship between (a) the energy (and, hence, the mass), (b) the radius and (c) the charge of an electron isĀ notĀ something God-given. What’s God-given are Maxwell’s equations, and so theĀ EeĀ = αe/reĀ = eP2/reĀ is just one of the many wonderful things that you can get out of Ā them.

So we found God’s ‘cut-off factor’ šŸ™‚ It’s equal to αeĀ ā‰ˆ 0.0073 = 7.3Ɨ10āˆ’3. So 7.3 thousands of… What? Well… Nothing. It’s just a pure ratio between the energy and the radius of an electron (if both are expressed in Planck units, of course). And so it determines the electron charge (again, expressed in Planck units). Indeed, we write:

eP = √αe

Really? Yes. JustĀ doĀ all these formulas:

ePĀ = √αeĀ ā‰ˆĀ āˆš0.0073Ā·1.9Ɨ10āˆ’18Ā coulombĀ ā‰ˆ 1.6Ā Ć—10āˆ’19 C

Just re-check itĀ withĀ all the known decimals: you’ll see it’s bang on. Let’s look at the EeĀ = meĀ = αe/reĀ ratio once again. What’s theĀ meaningĀ of it? Let’s first calculate the value of reĀ and me,Ā i.e. the electron radius and electron mass expressed in Planck units. It’s equal to the classical electron radius divided by the Planck length, and then the same for the mass, so we get the following thing:

reĀ ā‰ˆ (2.81794Ɨ10āˆ’15Ā m)/(1.6162Ɨ10āˆ’35Ā m) = 1.7435Ɨ1020Ā 

meĀ ā‰ˆ (9.1Ɨ10āˆ’31Ā kg)/(2.17651Ɨ10āˆ’8 kg) = 4.18Ɨ10āˆ’23

αeĀ = (4.18Ɨ10āˆ’23)Ā·(1.7435Ɨ1020) ā‰ˆ 0.0073

It works like a charm, but what does it mean? Well… It’s just a ratio between two physical quantities, and the scaleĀ you use to measure those quantities matters very much. We’ve explained that the Planck mass is a rather large unit at the atomic scale and, therefore, it’s perhaps not quite appropriate to use it here. In fact, out of the many interesting expressions for αe, I should highlight the following one:

αeĀ = e2/(ħ·c) ā‰ˆ (1.60217662Ɨ10āˆ’19 C)2/(4πε0Ā·[(1.054572Ɨ10āˆ’34 NĀ·mĀ·s)Ā·(2.998Ɨ108 m/s)])Ā ā‰ˆ 0.0073 once more šŸ™‚

Note that the elementary charge e is actually equal to qe/4πε0, which is what I am using in the formula. I know that’s confusing, but it what it is. As for the units, it’s a bit tedious to write it all out, but you’ll get there. Note that ε0Ā ā‰ˆ 8.8542Ɨ10āˆ’12Ā C2/(NĀ·m2) so… Well… All the units do cancel out, and we get a dimensionless number indeed, which is what αeĀ is.

The point is: this expression links αeĀ to the the de BroglieĀ relation (p =Ā h/Ī»), with Ī» the wavelengthĀ that’s associated with the electron. Of course, because of the Uncertainty Principle, we know we’re talking some wavelengthĀ rangeĀ really, so we should write the de Broglie relation asĀ Ī”p = hĀ·Ī”(1/Ī»). Now, that, in turn, allows us to try to work out the Bohr radius, which is the other ‘dimension’ we associate with an electron. Of course, now you’ll say: why would you do that. Why would you bring in the de BroglieĀ relation here?

Well… We’re talking energy, and so we have the Planck-EinsteinĀ relation first: the energy of some particle can always be written as the product of hĀ and some frequencyĀ f: E = hĀ·f. The only thing thatĀ de Broglie relation adds is the Uncertainty Principle indeed: the frequencyĀ fĀ will be some frequency range, associated with someĀ momentumĀ range, and so that’s what the Uncertainty Principle really says. I can’t dwell too much on that here, because otherwise this post would become a book. šŸ™‚ For more detail, you can check out one of my many posts on the Uncertainty Principle. In fact, the one I am referring to here has Feynman’s calculation of the Bohr radius, so I warmly recommend you check it out. The thrust of the argument is as follows:

  1. If we assume that (a) an electron takes some space – which I’ll denote by rĀ šŸ™‚ – and (b) that it has some momentum p because of its mass m and its velocity v, then the Ī”xĪ”p = ħ relation (i.e. the Uncertainty Principle in its roughest form) suggests that the order of magnitude of r and p should be related in the very same way. Hence, let’s just boldly write r ā‰ˆ ħ/p and see what we can do with that.
  2. We know that the kinetic energy of our electron equals mv2/2, which we can write as p2/2m so we get rid of the velocity factor.Well… Substituting our p ā‰ˆ ħ/r conjecture, we get K.E. = ħ2/2mr2. So that’s a formula for the kinetic energy. Next is potential.
  3. TheĀ formula for the potential energy is U = q1q2/4πε0r12. Now, we’re actually talking about the size of an atomĀ here, so one charge is the proton (+e) and the other is the electron (–e), so the potential energy is U = P.E. = –e2/4πε0r, with rĀ the ā€˜distance’ between the proton and the electron—so that’s the Bohr radius we’re looking for!
  4. We can now write the total energy (which I’ll denote by E, but don’t confuse it with the electric field vector!) asĀ E = K.E. + P.E. =  ħ2/2mr2 – e2/4πε0r. Now,Ā the electron (whatever it is) is, obviously, in some kind of equilibrium state. Why is that obvious? Well… Otherwise our hydrogen atom wouldn’t or couldn’t exist. šŸ™‚ Hence, it’s in some kind of energy ā€˜well’ indeed, at the bottom. Such equilibrium point ā€˜at the bottom’ is characterized by its derivative (in respect to whatever variable) being equal to zero. Now, the only ā€˜variable’ here isĀ rĀ (all the other symbols are physical constants), so we have to solve for dE/dr = 0. Writing it all out yields:Ā dE/dr = –ħ2/mr3Ā + e2/4πε0r2Ā = 0 ⇔ r =Ā 4πε0ħ2/me2
  5. We can now put the values in:Ā r =Ā 4πε0h2/me2Ā = [(1/(9Ɨ109) C2/NĀ·m2)Ā·(1.055Ɨ10–34Ā JĀ·s)2]/[(9.1Ɨ10–31Ā kg)Ā·(1.6Ɨ10–19Ā C)2]Ā = 53Ɨ10–12Ā m = 53 pico-meter (pm)

Done. We’re right on the spot.Ā The Bohr radius is, effectively, about 53 trillionthsĀ of a meter indeed!

Phew!

Yes… I know… Relax. We’re almost done. You should now be able to figure out why the classical electron radius and the Bohr radius can also be related to each other through the fine-structure constant. We write:

me = α/re = α/α2r = 1/αr

So we get that α/reĀ =Ā 1/αr and, therefore, we get re/r = α2, which explains why α is also equal to the so-called junction number, or the coupling constant, for an electron-photon coupling (see my post on the quantum-mechanical aspects of the photon-electron interaction). It gives a physical meaning to the probability (which, as you know, is the absolute square of the probability amplitude) in terms of the chance of a photon actually ‘hitting’ the electron as it goes through the atom. Indeed, the ratio of the Thomson scattering cross-section and the Bohr size of the atom should be of the same order asĀ re/r, and so that’s α2.

[Note: To be fully correct and complete, I should add that the coupling constant itself is not α2Ā but √α = eP. Why do we have this square root? You’re right: the fact that the probability is the absolute squareĀ of the amplitude explains one square root (√α2Ā = α), but not two. The thing is: the photon-electron interaction consists of twoĀ things. First, the electron sort of ‘absorbs’ the photon, and then it emits another one, that has the same or a different frequency depending on whether or not the ‘collision’ was elastic or not. So if we denote the coupling constant as j, then the whole interaction will have a probability amplitude equal to j2. In fact, theĀ value which Feynman uses in his wonderful popular presentation of quantum mechanics (The Strange Theory of Light and Matter), is āˆ’Ī± ā‰ˆ āˆ’0.0073. I am not quite sure why the minus sign is there. It must be something with the angles involved (the emitted photon will not be following the trajectory of the incoming photon) or, else, with the special arithmetic involved in boson-fermion interactions (we add amplitudes when bosons are involved, butĀ subtractĀ amplitudes when it’s fermions interacting.Ā I’ll probably find out once I am true through Feynman’s third volume ofĀ Lectures, which focus on quantum mechanics only.]

Finally, the last bit of unexplained ‘magic’ in the fine-structure constant is that the fine-structure constant (which I’ve started to write as α again, instead of αe) also gives us the (classical) relative speed of an electron, so that’s its speed as it orbits around the nucleus (according to the classical theory, that is), so we write

α = v/c = β

I should go through the motions here – I’ll probably do so in the coming days – but you can see we must be able to get it out somehow from all what we wrote above. See how powerfulĀ ourĀ Uelect  ∼ e2/a relation really is? It links the electron, charge, its radius and its energy, and it’s all we need to all the rest out of it: its mass, its momentum, its speed and – through the Uncertainty Principle – the Bohr radius, which is the size of the atom.

We’ve come a long way. This is truly a milestone. We’ve taken the magic out of God’s number—to some extent at least. šŸ™‚

You’ll have one last question, of course: if proportionality constants are all about theĀ scaleĀ in which weĀ measureĀ the physical quantities on either side of an equation, is there some way the fine-structure constant would come out differently? That’s the same as asking: what if we’d measure energy in units that are equivalent to the energy of an electron, and the radius of our electron just as… Well… What if we’d equate our unit of distance with the radius of the electron, so we’d write re = 1? What would happen to α? Well…Ā I’ll let you figure that one out yourself. I am tired and so I should go to bed now. šŸ™‚

[…] OK. OK. Let me tell you. It’s not that simple here. All those relationships involving α, in one form or the other, are very deep. They relate a lot of stuff to a lot of stuff, and we can appreciate that only when doing a dimensional analysis. A dimensional analysis of the EeĀ = αe/reĀ = eP2/rĀ yields [eP2/r] = C2/m on the right-hand side and [Ee] = J = NĀ·mĀ on the left-hand side. How can we reconcile both? The coulomb is an SI base unitĀ , so we can’t ‘translate’ it into something with N and m. [To be fully correct, for some reason, theĀ ampĆØreĀ (i.e. coulombĀ per second) was chosen as an SI base unit, but they’re interchangeable in regard to their place in the international system of units: they can’t be reduced.] So we’ve got a problem. Yes. That’s where we sort of ‘smuggled’ the 4πε0 factor in when doing our calculations above. That ε0 constant is, obviously, not ‘as fundamental’ as cĀ or α (just think of the cāˆ’2Ā = ε0μ0 relationship to understand what I mean here) but, still, it was necessary to make the dimensions come out alright: we need the reciprocalĀ dimensionĀ of ε0, i.e. (NĀ·m2)/C2, to make the dimensional analysis work.Ā We get: (C2/m)Ā·(NĀ·m2)/C2Ā = NĀ·m = J, i.e.Ā joule, so that’s the unit in which we measure energy or – using the E = mc2Ā equivalence – mass, which is the aspect of energy emphasizing itsĀ inertia.

So the answer is: no. Changing units won’t change alpha. So all that’s left is to play with it now. Let’s try to do that. Let me first plot that EeĀ = meĀ = αe/re = 0.00729735256/re:

graph 3Unsurprisingly, we find theĀ pivotĀ point of this curve is at the intersection of the diagonal and the curve itself, so that’s at the (0.00729735256,Ā 0.00729735256) point, where slopes are ± 1, i.e. plus or minus unity.Ā What does this show? Nothing much. What?Ā I can hear you: I should be excited because… Well… Yes! Think of it. If youĀ would have to chose a cut-off point, you’d chose this one, wouldn’t you? šŸ™‚ Sure, you’re right. How exciting! Let me show you. Look at it! It proves that God thinks in terms of logarithms. He has chosen α such that ln(E) = ln(α/r) = lnα – lnrĀ = lnα – lnrĀ = 0, so ln α = lnr and, therefore, α = r. šŸ™‚

Huh? Excuse me?

I am sorry. […] Well… I am not, of course… šŸ™‚ I just wanted to illustrate the kind of exercise some people are tempted to do. It’s no use. The fine-structure constant is what it is: it sort ofĀ summarizesĀ an awful lot of formulas. It basically shows what Maxwell’s equation imply in terms of theĀ structureĀ of an atom defined as a negativeĀ charge orbiting around some positive charge. It shows we can get calculate everything as a function of something else, and that’s what the fine-structure constant tells us: it relates everything to everything. However, when everything is said and done, the fine-structure constant shows us two things:

  1. Maxwell’s equations are complete: we canĀ construct a complete model of the electron and the atom, which includes: the electron’s energy and mass, its velocity, its own radius, and the radius of the atom. [I might have forgotten one of the dimensions here, but you’ll add it. :-)]
  2. God doesn’t want our equations to blow up. Our equations are all correct but, in reality, there’s a cut-off factor that ensures we don’t go to the limit with them.

So the fine-structure constant anchors our world, so to speak. In other words: of all the worlds that are possible, we live in this one.

[…] It’s pretty good as far as I am concerned. Isn’t it amazing that our mind is able to justĀ graspĀ things like that? I know my approach here is pretty intuitive, and with ‘intuitive’, I mean ‘not scientific’ here. šŸ™‚ Frankly, I don’t like the talk about physicists “looking into God’s mind.” I don’t think that’s what they’re trying to do. I think they’re just trying to understand the fundamentalĀ unityĀ behind it all. And that’s religion enough for me. šŸ™‚

So… What’s the conclusion? Nothing much. We’ve sort of concluded our description of the classical world… Well… Of its ‘electromagnetic sector’ at least. šŸ™‚ That sector can be summarized in Maxwell’s equations, which describe an infinite world of possible worlds. However, God fixed three constants:Ā h,Ā cĀ and α. So we live in a world that’s defined by this Trinity of fundamental physical constants. Why is it not two, or four?

My guts instinct tells me it’s because we live in three dimensions, and so there’s three degrees of freedom really. But what about time? Time is the fourth dimension, isn’t it? Yes. But time is symmetric in the ‘electromagnetic’ sector: we can reverse the arrow of time in our equations and everything still works. TheĀ arrow of timeĀ involves other theories: statistics (physicists refer to it as ‘statistical mechanics‘) and the ‘weak force’ sector, which I discussed when talking about symmetries in physics. So… Well… We’re not done. God gave us plenty of other stuff to try to understand. šŸ™‚

Field energy and field momentum

This post goes to the heart of the E = mc2, equation. It’sĀ kindaĀ funny, because Feynman just compresses all of it in a sub-section of hisĀ Lectures. However, as far as I am concerned, I feel it’s a very crucial section. Pivotal, I’d say, which would fit with its place in all of the 115 LecturesĀ that make up the three volumes, which is sort of mid-way, which is where we are here.Ā So let’s get go for it. šŸ™‚

Let’s first recall what we wrote about the Poynting vector S, which we calculate from the magnetic and electric field vectors E and B by taking their cross-product:

S formula

This vector represents the energy flow, per unit area and per unit time, in electrodynamical situations. If E and/or BĀ are zero (which is the case in electrostatics, for example, because we don’t have magnetic fields in electrostatics), then S is zero too, so there is no energy flow then. That makes sense, because we have no moving charges, so where would the energy go to?

I also made it clear we should think of S as something physical, by comparing it to the heat flow vectorĀ h, which we presented when discussing vector analysis and vector operators. The heat flow out of a surface element daĀ is the area times the component ofĀ hĀ perpendicular to da, so that’s (h•n)Ā·da = hnĀ·da. Likewise, we can writeĀ (S•n)Ā·da = SnĀ·da. The units of S and h are also the same:Ā joule per second and per square meterĀ or, using the definition of theĀ wattĀ (1 W = 1 J/s), in watt per square meter.Ā In fact, if you google a bit, you’ll find that both hĀ and S are referred to as aĀ flux density:

  1. The heat flow vector hĀ is the heat flux densityĀ vector, from which we get the heat flux through an area through the (h•n)Ā·da = hnĀ·daĀ product.
  2. The energy flow SĀ is the energy flux density vector, from which we get the energy flux through the (S•n)Ā·da = SnĀ·daĀ product.

So that should be enough as an introduction to what I want to talk about here. Let’s first look at the energy conservation principle once again.

Local energy conservation

In a way, you can look atĀ my previous postĀ as being all about the equation below, which we referred to as the ‘local’ energy conservation law:

energy flux

Of course, it is notĀ theĀ completeĀ energy conservation law. The local energy is not only in the field. We’ve got matter as well, and so that’s what I want to discuss here: we want to look at the energy in the field as well as the energy that’s in the matter. Indeed, field energy is conserved, and then it isn’t: if the field is doing work on matter, or matter is doing work on the field, then… Well… Energy goes from one to the other, i.e. from the field to the matter or from the matter to the field. So we need to include matter in our analysis, which we didn’t do in our last post. Feynman gives the following simple example: we’re in a dark room, and suddenly someone turns on the light switch. So now the room is full of field energy—and, yes, I just mean it’s not dark anymore. :-). So that means someĀ matter out thereĀ must have radiated its energy out and, in the process, it must have lost the equivalent mass of that energy. So, yes, we had matter losing energy and, hence, losing mass.

Now, we know that energy and momentum are related. Respecting and incorporating relativity theory, we’ve got two equivalentĀ formulas for it:

  1. E2Ā āˆ’ p2c2Ā = m02c4
  2. pcĀ = EĀ·(v/c) ⇔ p = vĀ·E/c2Ā = mĀ·v

The EĀ = mc2Ā and m = Ā·m0Ā·(1āˆ’v2/c2)āˆ’1/2Ā formulas connect both expressions. So we canĀ look at it in either of two ways. We couldĀ useĀ the energy conservation law, but Feynman prefers the conservation of momentum approach, so let’s see where he takes us. If the field has some energyĀ (and, hence, some equivalent mass) per unit volume, and if there’s someĀ flow, so if there’s someĀ velocityĀ (which there is: that’s what our previous post was all about), then it will have a certain momentumĀ per unit volume. [Remember: momentum isĀ massĀ timesĀ velocity.] That momentum will have aĀ direction, so it’s a vector, just like p = mv. We’ll write it as g, so we define g as:

g is the momentum of the field per unit volume.

What units would we express it in? We’ve got a bit of choice here. For example, because we’re relating everything to energy here, we may want to convert our kilogram into eV/c2Ā or J/c2Ā units, using the mass-energy equivalence relation EĀ = mc2. Hmm… Let’s first keep the kg as a measure of inertia though. So we write: [g] = [m]Ā·[v]/m3Ā = (kgĀ·m/s)/m3. Hmm… That doesn’t show it’s energy, so let’s replace the kg with a unit that’s got newton and meter in it, cf. the F = ma law. So we write:Ā [g] = (kgĀ·m/s)/m3Ā =Ā (kg/s)/m2Ā = [(NĀ·s2/m)/s]/m2Ā =Ā NĀ·s/m3. Well… OK. The newtonĀ·second is the unit of momentum indeed, and we can re-write it including the joule (1 J = 1 NĀ·m), so then we get [g] = (JĀ·s/m4), so what’s that? Well… Nothing much. However, I do note it happens to be the dimension of S/c2, so that’s [S/c2] = [J/(sĀ·m2)]Ā·(s2/m2) =Ā (JĀ·s/m4). šŸ™‚ Let’s continue the discussion.

Now, momentum is conserved, and eachĀ componentĀ of it is conserved. So let’s look at the x-direction. We should have something like:

formula

If you look at this carefully, you’ll probably say: “OK. I understood the thing with the dark room and light switch. Mass got converted into field energy, but what’s that second term of the left?”

Good. Smart. RightĀ remark. Perfect. […] Let me try to answer the question. While all of the quantities above are expressedĀ per unit volume, we’re actually looking at the sameĀ infinitesimal volume element here, so the example of the light switch is actually an example of a ‘momentum outflow’, so it’s actually an example of that second term of the left-hand side of the equation above kicking in! šŸ™‚

Indeed, the first term just sort of reiterates the mass-energy equivalence: the energy that’s in the matter can become field energy, so to speak, in our infinitesimal volume element itself, and vice versa. But if it doesn’t, then it should get out and, hence, become ‘momentum outflow’. Does that make sense? No?

Hmm… What to say? You’ll need to look at that equation a couple of times more, I guess. :-/ But I need to move on, unfortunately. [Don’t get put off when I say things like this: I am basically talking to myself, so it means I’ll need to re-visit this myself. :-/]

Let’s look at all of the three terms:

  1. The left-hand side (i.e. the time rate-of-change of the momentum of matter) isĀ easy. It’s just the force on it, which we know is equal to F =Ā q(E+vƗB). Do we know that? OK… I’ll admit it.Ā Sometimes it’s easy to forget where we are in an analysis like this, but so we’re looking at the electromagnetic force here. šŸ™‚ As we’re talking infinitesimals here and, therefore, chargeĀ densityĀ rather than discreteĀ charges, we should re-write this as the force per unit volume which is ρE+jƗB. [This is an interesting formula which I didn’t use before, so you should double-check it. :-)]
  2. The first term on the right-hand side should be equally obvious, or… Well… Perhaps somewhat less so. But with all my rambling on the Uncertainty PrincipleĀ and/or the wave-particle duality, it should make sense. If we scrap the second term on the right-hand side, we basically have an equation that is equivalent to the E = mc2Ā equation. No? Sorry. Just look at it, again and again. You’ll end up understanding it. šŸ™‚
  3. So it’s that second term on the right-hand side. What the hell does thatĀ say? Well… I could say: it’s the local energy or momentum conservation law. If the energy or momentum doesn’t stay in, it has to go out. šŸ™‚ But that’s not very satisfactory as an answer, of course. However, please just go along with thisĀ ‘temporary’ answer for a while.

So what isĀ that second term on the right-hand side? As we wrote it, it’s an x-component – or, let’s put it differently, it is or was part of the x-component of the momentum density – but, frankly, we should probably allow it to go out in any direction really, as the only constraint on the left-hand side is a per secondĀ rate of change of something. Hence, Feynman suggest to equate it to something like this:

general

What a, b and c? The components of some vector? Not sure. We’re stuck. This pieceĀ reallyĀ requiresĀ veryĀ advanced math. In fact, as far as I know, this is the onlyĀ time where Feynman says: “Sorry. This is too advanced. I’ll just give you the equation. Sorry.” So that’s what he does. He explains the philosophyĀ of the argument, which is the following:

  1. On the left-hand side, we’ve got the time rate-of-change of momentum, so that obeys the F = dp/dt = d(mv)/dt law, with the force F,Ā per unit volume, being equal to F(unit volume) = ρE+jƗB.
  2. On the right-hand side, we’ve got something that can be written as:

general 2

So we’d need to find a way to ρE+jƗBĀ in terms of EĀ andĀ B only – eliminating ρ andĀ jĀ by using Maxwell’s equations or whatever other trick  – and then juggle terms and make substitutions to get it into a form that looks like the formula above, i.e. the right-hand side of that equation. But so Feynman doesn’t show us how it’s being done. He just mentions some theorem in physics, which says that the energy that’s flowing through a unit area per unit time divided byĀ c2 – so that’s E/c2Ā per unit area and per unit time – must be equal to the momentum per unit volume in the space, so we write:

g = S/c2

HeĀ illustratesĀ the general theorem that’s used to get the equation above by giving two examples:

example theorem

OK. Two good examples. However, it’s still frustrating toĀ notĀ see how we get the g = S/c2Ā in the specificĀ context of the electromagnetic force, so let’s do a dimensional analysis at least. In my previous post, I showed thatĀ the dimension ofĀ S mustĀ be J/(m2Ā·s), so [S/c2] = [J/(m2Ā·s)]/(m2/s2) = [NĀ·m/(m2Ā·s)]Ā·(s2/m2) = [NĀ·s/m3]. Now, we know that the unit of mass is 1 kg = N/(m/s2). That’s just the force law: a force of 1 newton will give a mass of 1 kg an acceleration of 1 m/s per second, so 1 N = 1 kgĀ·(m/s2). So theĀ [NĀ·s/m3] dimension is equal to [kgĀ·(m/s2)Ā·s/m3] = [(kgĀ·(m/s)/m3] =Ā [(kgĀ·(m/s)]/m3, which is the dimension of momentum (p = mv) per unit volume, indeed.Ā So, yes, the dimensional analysis works out, and it’s also in line with theĀ p = vĀ·E/c2Ā = mĀ·v equation, but… Oh… We did a dimensional analysis already, where we also showed that [g]Ā = [S/c2] = (JĀ·s/m4). Well… In any case… It’s a bit frustrating to notĀ see the detail here, but let us note the the Grand ResultĀ once again:

The Poynting vector S gives us the energy flow as well as the momentum density gĀ = S/c2.

But what does it all mean, really? Let’s go through Einstein’s illustration of the principle. That will help us a lot. Before we do, however, I’d like to note something. I’ve always wondered a bit about that dichotomy between energy and momentum. Energy is force times distance: 1Ā jouleĀ is 1Ā newtonĀ Ć— 1Ā meterĀ indeed (1 J = 1 NĀ·m). Momentum is force times time, as we can express it in NĀ·s. Planck’s constant hĀ combines all three in the dimension ofĀ action, which isĀ forceĀ timesĀ distanceĀ timesĀ time: hĀ ā‰ˆĀ 6.6Ɨ10āˆ’34Ā NĀ·mĀ·s, indeed. I like that unity. In this regard, you should, perhaps, quickly review that post in which I explain that hĀ isĀ the energy per cycle, i.e. per wavelength or per period, of a photon, regardless of its wavelength. So it’s really something very fundamental.

We’ve got something similar here: energy and momentum coming together, and being shown as one aspect of the same thing: some oscillation. Indeed, just see what happens with the dimensions when we ‘distribute’ the 1/c2Ā factor on the right-hand side over the two sides, so we write:Ā cĀ·gĀ = S/c and work out the dimensions:

  1. [cĀ·g ]Ā = (m/s)Ā·(NĀ·s)/m3Ā = N/m2Ā = J/m3.
  2. [S/c] =Ā (s/m)Ā·(NĀ·m)/(sĀ·m2) = N/m2Ā = J/m3.

Isn’t that nice? Both sides of the equation now have a dimension like ‘the force per unit area’, or ‘the energy per unit volume’. To get that, we just re-scaled g and S, by c and 1/c respectively. As far as I am concerned, this shows an underlying unity we probably tend to mask with our ‘related but different’ energy and momentum concepts. It’s like E and B: I just love it we can write them together in our Poynting formula SĀ = ε0c2EƗB. In fact, let me show something else here, which you should think about. You know that c2Ā = 1/(ε0μ0), so we can write SĀ also as S =Ā EƗB/μ0. That’s nice, but what’s nice too is the following:

  1. S/c = cĀ·gĀ = ε0cEƗBĀ = EƗB/μ0c
  2. S/g = c2 = 1/(ε0μ0)

So, once again, Feynman may feel the Poynting vector is sort of counter-intuitive when analyzing specific situations but, as far as I am concerned, I feel the Poyning vector makes things actuallyĀ easierĀ to understand. Instead of two E and B vectors, and two concepts to deal with ‘energy’ (i.e. energy and momentum), we’re sort of unifying things here. In that regard – i.e in regard of feeling we’re talking the same thing really – I’d really highlight the S/g = c2 = 1/(ε0μ0) equation. Indeed, the universal constantĀ cĀ acts just like the fine-structure constant here: it links everything to everything. šŸ™‚

And, yes, it’s also about time we introduce the so-called principle of least action to explain things, becauseĀ action, as a concept, combines force, distance and time indeed, so it’s a bit more promising than just energy, of just momentum. Having said that, you’ll see in the next section that it’s sometimes quite useful to have the choice between one formula or the other. But… Well…Ā Enough talk. Let’s look at Einstein’s car.

Einstein’s car

Einstein’s car is a wonderful device: it rolls without any friction and it moves with a little flashlight. That’s all it needs. It’s pictured below. šŸ™‚ So the situation is the following: the flashlight shoots some light out from one side, which is then stopped at the opposite end of the car. When the light is emitted, there must be some recoil. In fact, we know it’s going to be equal to 1/c times the energy because all we need to do is apply theĀ pcĀ = EĀ·(v/c) formula forĀ v = c, so we know that p = E/c. Of course, this momentum now needs to move Einstein’s car. It’s frictionless, so it should work, but still… The car has some mass M, and so that will determine its recoil velocity: v = p/M. We just apply the general p = mv formula here, and v is notĀ equal toĀ c here, of course! Of course, then the light hits the opposite end of the car and delivers the same momentum, so that stops the car again. However, itĀ didĀ move over some distance x = vt. So we could flash our light again and get to wherever we want to get. [Never mind the infinite accelerations involved!] So… Well… Great! Yes, but Einstein didn’t like this car when he first saw it. In fact, he still doesn’t like it, because he knows it won’t take you very far. šŸ™‚

Einsteins' car

The problem is that we seem to be moving the center of gravity of this car by fooling around on the inside only. Einstein doesn’t like that. He thinks it’s impossible. And he’s right of course. The thing is: the center of gravity didĀ notĀ change. What happened here is that we’ve got someĀ blob of energy, and so that blob has some equivalent mass (which we’ll denote by U/c2), and so that equivalent mass moved all the way from one side to the other, i.e. over the length of the car, which we denote by L. In fact, it’s stuff like this that inspired the whole theory of the field energy and field momentum, and how it interacts withĀ matter.

What happens here is like switching the light on in the dark room: we’ve got matter doing work on the field, and so matter loses mass, and the field gains it, through its momentum and/or energy. To calculate how much, we could integrate S/cĀ or cĀ·gĀ over the volume of our blob, and we’d get something in jouleĀ indeed, but there’s a simpler way here. The momentum conservation says that the momentum of our car and the momentum of our blob must be equal, so if T is the time that was needed for our blob to go to the other side – and so that’s, of course, also the time during which our car was rolling – then MĀ·v = MĀ·x/T must be equal to (U/c2)Ā·cĀ =Ā (U/c2)Ā·L/T. The 1/T factor on both sides cancel, so we write:Ā MĀ·x = (U/c2)Ā·L.Ā Now, what is x? Yes. In case you were wondering, that’s what we’re looking for here. šŸ™‚ Here it is:

x = vT = vL/c = (p/M)Ā·(L/c) = [U/c)/M]Ā·(L/c) = (U/c2)Ā·(L/M)

So what’s next? Well… Now we need to show that the center-of-mass actually didĀ notĀ move with this ‘transfer’ of the blob. I’ll leave the math to you here: it should all work out. And you can also think through the obvious questions:

  1. Where is the energy and, hence, the mass of our blob after it stops the car? Hint: think about excited atoms and imagine they might radiate some light back. šŸ™‚
  2. As the car did move a little bit, we should be able to move it further and further away from its center of gravity, until the center of gravity is no longer in the car. Hint: think about batteries and energy levels going down while shooting light out. It just won’t happen. šŸ™‚

Now, what about a blob of light going from the top to the bottom of the car? Well… That involves the conservation ofĀ angularĀ momentum: we’ll have more mass on the bottom, but on a shorter lever-arm, soĀ angularĀ momentum is being conserved. It’s aĀ veryĀ good question though, and it led Einstein to combine the center-of-gravity theorem with the angular momentum conservation theorem to explain stuff like this.

It’s all fascinating, and one can think of a great many paradoxes that, at first, seem to contradict the Grand Principles we used here, which means that they would contradict all that we have learned so far. However, a careful analysis of those paradox reveals that they are paradoxes indeed:Ā propositions which soundĀ true but are, in the end,Ā self-contradictory. In fact, when explaining electromagnetism over his variousĀ Lectures, Feynman tasks his readers with a rather formidable paradox when discussing the laws of induction, he solves it here, ten chapters later, after describing what we described above. You can busy yourself with it but… Well… I guess you’ve got something better to do. If so, just take away the key lesson: there’s momentum in the field, and it’s also possible to build upĀ angularĀ momentum in a magneticĀ field and, if you switch it off, the angular momentum will be given back, somehow, as it’s stored energy.

That’s also why the seemingly irrelevant circulation of SĀ we discussed in my previous post, where we had a charge next to an ordinary magnet, and where we found that there was energy circulating around, is not so queer. The energy is there, in the circulating field, and it’sĀ real. As real as can be. šŸ™‚

crazy

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

The energy of fields and the Poynting vector

For some reason, I always thought that Poynting was a Russian physicist, like Minkowski. He wasn’t. I just looked it up. Poynting was anĀ Englishman, born near Manchester, and he teached in Birmingham. I should have known. Poynting is a very English name, isn’t it? My confusion probably stems from the fact that it was someĀ Russian physicist,Ā Nikolay Umov, who first proposed the basic concepts we are going to discuss here, i.e. the speed and direction of energy itself, or its movement. And as I am double-checking, I just learned that Hermann Minkowski is generally considered to be German-Jewish, not Russian. Makes sense. With Einstein and all that. His personal life story is actually quite interesting. You should check it out. šŸ™‚

Let’s go for it. We’ve done a few posts on the energy in the fields already, but all in the contexts of electrostatics. Let me first walk you through the ideas we presented there.

The basic concepts: force, work, energy and potential

1.Ā A charge q causes an electric field E, and E‘sĀ magnitude E is a simple function of the charge (q) and its distance (r) from the point that we’re looking at, which we usually write as P = (x, y, z). Of course, the origin of our reference frame here is q. The formula is the simple inverse-square law that you (should) know: E ∼ q/r2, and the proportionality constant is just Coulomb’s constant, which I think you wrote as keĀ in your high-school days and which, as you know, is there so as to make sure the units come out alright. So we could just writeĀ E = keĀ·q/r2. However, just to makeĀ sure it doesĀ notĀ look like a piece of cake šŸ™‚ physicists writeĀ the proportionality constant as 1/4πε0, so we get:

E 3

Now, the field is the force on any unit charge (+1) we’d bring to P. This led us to think of energy,Ā potentialĀ energy, because… Well… You know: energy is measured by work, so that’s some force acting over some distance. The potential energy of a charge increases if we move it againstĀ the field, so we wrote:

formula 1

Well… We actually gave the formula below in that post, so that’s the work done per unit charge.Ā To interpret it, you just need to remember that F = qE, which is equivalent to saying that E is the force per unit charge.

unit chage

As for the F•ds or E•ds product in the integrals, that’s a vector dot product, which we need because it’s only the tangential component of the force that’s doing work, as evidenced by the formula F•ds =Ā |F|Ā·|ds|Ā·cosĪø = FtĀ·ds, and as depicted below.

illustration 1

Now, thisĀ allowed us to describe the field in terms of the (electric)Ā potential Φ and the potential differencesĀ between two points, like the points a and b in the integral above. We have to chose some reference point, of course, someĀ P0Ā defining zero potential, which is usually infinitely far away. So we wrote our formula for the work that’s being done on a unit charge, i.e. W(unit) as:

potential

2.Ā The world is full of charges, of course, and so we need to add all of their fields. But so now you need a bit of imagination. Let’s reconstruct the world by moving all charges out, and then we bring them back one by one. So we take q1Ā now, and we bring it back into the now-empty world. NowĀ that does notĀ require any energy, because there’s no field to start with. However, when we take our second chargeĀ q2, we will be doing work as we move it against the field or, if it’s an opposite charge, we’ll be taking energy out of the field.Ā Huh?Ā Yes. Think about it. All is symmetric.Ā Just to make sure you’re comfortable with every step we take, let me jot down the formula for the force that’s involved. It’s just theĀ CoulombĀ force of course:

Coulomb's law

F1Ā is the force on charge q1, andĀ F2Ā is the force on charge q2. Now, q1Ā and q2. may attract or repel each other but the forces will alwaysĀ be equal and opposite. The e12Ā vector makes sure the directions and signs come out alright, as it’s the unit vector from q2Ā to q1Ā (not from q1Ā to q2, as you might expect when looking at the order of the indices). So we would need to integrate this forĀ rĀ going from infinity to… Well… The distance betweenĀ q1Ā and q2 – wherever they end up as we put them back into the world – so that’s what’s denoted by r12. Now I hate integrals too, but this is an easy one. Just note that ∫ rāˆ’2dr = 1/r and you’ll be able to figure out that what I’ll write now makes sense (if not, I’ll do a similar integral in a moment): the work done in bringing two charges together from a large distance (infinity) is equal to:

U 1So now we should bring in q3Ā and then q4, of course. That’s easy enough.Ā Bringing the first two charges into that world we had emptied took a lot of time, but now we can automate processes. Trust me: we’ll be done in no time. šŸ™‚ We just need to sum over all of theĀ pairsĀ of chargesĀ qiĀ andĀ qj. So we writeĀ the total electrostatic energy UĀ as the sum of the energies of all possible pairs of charges:

U 3

Huh?Ā Can we do that?Ā I mean… Every new charge that we’re bringing in here changes the field, doesn’t it? It does. But it’s the magic of the superposition principle at work here. Our third charge q3Ā is associated with two pairs in this formula. Think of it: we’ve got theĀ q1q3Ā and theĀ q2q3Ā combination, indeed. Likewise, our fourh chargeĀ q4Ā is to be paired up withĀ three charges now: q1,Ā q1Ā andĀ q3. This formula takes care of it, and theĀ ‘all pairs’ mentionĀ under the summationĀ sign (Ī£) reminds us we should watch we don’t double-count pairs:Ā theĀ q1q3Ā and q3q1Ā combination, for example, count for one pair only, obviously. So, yes, we write ‘all pairs’ instead of the usual i, j subscripts. But then, yes, this formula takes care of it. We’re done!

Well… Not really, of course. We’ve still got some way to go before I can introduce the Poynting vector. šŸ™‚ However, to make sure you ‘get’ the energy formula above, let me insert an extremely simple diagram so you’ve got a bit of a visual of what we’re talking about.

U system

3.Ā Now, let’s take a step back. We just calculated the (potential)Ā energy of the world (U), which is great. But perhaps we should also be interested in the world’sĀ potential Φ, rather than its potential energy U. Why? Well, we’ll want to know what happens when we bring yet another charge in—from outer space or so. šŸ™‚ And so then it’s easier to know the world’s potential, rather than its energy, because we can calculate the field from it using the E =Ā āˆ’āˆ‡Ī¦ formula.Ā So let’s de- and re-construct the world once again šŸ™‚ but now we’ll look at what happens with the field and the potential.

We know our first charge created a field with a field strength we calculated as:

E 3

So, when bringing in our second charge, we can use our Φ(P) integral to calculate the potential:

potential

[Let me make a note here, just for the record. You probablyĀ think I am being pretty childish when talking about my re-construction of the world in terms of bringing all charges out and then back in again but, believe me, there will be a lot of confusion when we’ll start talking about the energy of oneĀ charge, and that confusion can be avoided, to a large extent, when you realize that the idea (I mean the concept itself, really—not its formula)Ā of a potential involves two charges really. Just remember: it’s theĀ firstĀ charge that causes the field (and, of course, anyĀ charge causes a field),Ā but calculating a potential only makes sense when we’re talking someĀ other charge.Ā Just make a mental note of it. You’ll be grateful to me later.]

Let’s nowĀ combine the integral and the formula for E above. Because you hate integrals as much as I do, I’ll spell it out: the antiderivative of the Φ(P) integral is ∫ q/(4πε0r2)Ā·dr. Now, let’s bring q/4πε0 out for a while so we can focus on solving ∫(1/r2)dr. Now, ∫(1/r2)drĀ is equal to –1/r + k, and so the whole antiderivative is –q/4πε0rĀ + k. Now, we integrate from r = āˆž to r, and so the definite integral is [–q/(4πε0)]Ā·[1/āˆž āˆ’ 1/r] = [–q/(4πε0)]Ā·[0 āˆ’ 1/r]Ā = q/(4πε0r). Let me present this somewhat nicer:

E 4

You’ll say: so what? Well… We’re done! The only thing we need to do now is add up the potentials of all of the charges in the world. So the formula for the potential Φ at a point which we’ll simply refer to as point 1, is:

P 1

Note that our index jĀ starts at 2, otherwise it doesn’t make sense: we’d have a division by zero for the q1/r11Ā term. Again, it’s an obvious remark, butĀ notĀ thinking about it can cause a lot of confusion down the line.

4.Ā Now, I am veryĀ sorry but I have to inform you that we’ll be talking charge densitiesĀ and all that shortly, rather than discreteĀ charges, so I have to give you the continuumĀ version of this formula, i.e. the formula we’ll use when we’ve got charge densities rather than individual charges. That sum above then becomes an infinite sum (i.e. an integral), and qjĀ becomes a variable which we write as ρ(2). [That’s totally in line with our index jĀ starts at 2, rather than from 1.] We get:

U 2

Just look at this integral, and try to understand it: we’re integrating over all of space – so we’re integrating the whole world, really šŸ™‚Ā ā€“ and the ρ(2)Ā·dV2Ā product in the integral is just the charge of an infinitesimally small volumeĀ of our world. So the whole integral is just the (infinite) sum of the contributions to the potential (at point 1) of all (infinitesimally small) charges that are around indeed. Now, there’s something funny here. It’s just a mathematical thing: we don’t need to worry about double-counting here. Why? We’re not having products of volumes here. Just make a mental note of it because it will be different in a moment.

Now we’re going to look at the continuum version for our energy formula indeed. Which energy formula? That electrostatic energy formula, which said thatĀ the total electrostatic energy UĀ as the sum of the energies of all possible pairs of charges:

U 3

Its continuum version is the following monster:

U 4

Hmm… What kind of integral is that? We’ve gotĀ two variables here: dV2Ā and dV1. Yes. And we’ve also got a 1/2 factor now, because we do notĀ want to double-count and, unfortunately, there is no convenient way of writing an integral like this that keeps track of the pairs. It’s a so-called double integral, but I’ll let you look up the math yourself. In any case, we can simplify this integral so you don’t need to worry about it too much. How do we simplify it? Well… Just look at that integral we got for Φ(1): we calculated the potential at point 1 by integratingĀ the ρ(2)Ā·dV2Ā product over all of space, so the integral above can be written as:

U 5But so thisĀ integral integrates the ρ(1)·Φ(1)Ā·dV1Ā product over all of space, so that’s over all points in space. So we can just drop the index and write the whole thing as the integral of ρ·Φ·dVĀ over all of space:

U 6

5. It’s time for the hat-trick now. The equation above is mathematically equivalent to the following equation:

U 7

Huh?Ā Yes. Let me make two remarks here. First on the math, the E =Ā āˆ’āˆ‡Ī¦ formula allows you to the integrand of the integral above asĀ E•EĀ =Ā (āˆ’āˆ‡Ī¦)•(āˆ’āˆ‡Ī¦) = (āˆ‡Ī¦)•(āˆ‡Ī¦). And then you may or may not remember that, when substitutingĀ E =Ā āˆ’āˆ‡Ī¦ in Maxwell’s first equation (āˆ‡ā€¢E = ρ/ε0), we got the following equality: ρ = ε0Ā·āˆ‡ā€¢(āˆ‡Ī¦) = ε0Ā·āˆ‡2Φ, so we can write ρΦ as ε0Ā·Ī¦Ā·āˆ‡2Φ. However, that still doesn’t show the two integrals are the same thing. The proof is actually rather involved, and so I’ll refer to that post I referred to, so you can check the proof there.

The second remark is much more fundamental. The two integrals are mathematically equivalent, but are they also physically? What do I mean with that? Well… Look at it. The second integral implies that we can look at (ε0/2)Ā·E•E = ε0E2/2 as an energy density, which we’ll denote by u, so we write:

D 6

Just to make sure you ā€˜get’ what we’re talking about here: u is the energy density in the little cube dV in the rather simplistic (and, therefore, extremely useful) illustration below (which, just like most of what I write above, I got from Feynman).

Capture

Now the question: what is theĀ realityĀ of that formula? Indeed, what we did when calculating U amounted to calculating theĀ Universe with some numberĀ U – and that’s kinda nice, of course! – but then what? Is u = ε0E2/2 anything real? Well… That’s what this post is about. So we’re finished with the introduction now. šŸ™‚

Energy density and energy flow in electrodynamics

Before giving you any more formulas, let me answer the question: there is no doubt, in the classical theory of electromagnetism at least, that the energy density u is somethingĀ very real. ItĀ hasĀ to be because of the charge conservation law. Charges cannot just disappear in space, to then re-appear somewhere else. The charge conservation law is written asĀ āˆ‡ā€¢j =Ā āˆ’āˆ‚Ļ/āˆ‚t, and that makes it clear it’s aĀ localĀ conservation law. Therefore, charges can only disappear and re-appear through some current. We write dQ1/dt = ∫ (j•n)Ā·da = āˆ’dQ2/dt, and here’s the simple illustration that comes with it:

charge flow

So we doĀ notĀ allow for any ‘non-local’ interactions here! Therefore, we say that, if energy goes away from a region, it’s because itĀ flowsĀ away through the boundaries of that region.Ā So that’s what the Poynting formulas are all about, and so I want to be clear on that from the outset.

Now, to get going with the discussion, I need to give you the formula for the energy density inĀ electrodynamics. Its shape won’t surprise you:

energy density

However, it’s just like the electrostatic formula: it takes quite a bit of juggling to get this from our electrodynamic equations, so, if you want to see how it’s done, I’ll refer you to Feynman. Indeed, I feel the derivation doesn’t matter all that much, because the formula itself is veryĀ intuitive: it’s really the thing everyone knows about a wave, electromagnetic or not: the energy in it is proportional to the square of its amplitude, and so that’s E•EĀ =Ā E2Ā and B•BĀ = B2. Now, you also know that the magnitudeĀ of B is 1/c of that of E, so cB = E, and so that explains the extra c2Ā factor in the second term.

The second formula is also very intuitive. Let me write it down:

energy flux

Just look at it: uĀ is the energy density, so that’s the amount of energy per unit volumeĀ at a given point, and so whatever flows out of that point must represent itsĀ time rate of change. As for the ā€“āˆ‡ā€¢S expression… Well… Sorry, I can’t keep re-explaining things: theĀ āˆ‡ā€¢ operator is the divergence, and so it give us the magnitude of a (vector) field’s source or sinkĀ at a given point. āˆ‡ā€¢CĀ is a scalar, and if it’sĀ positive in a region, then that region is a source. Conversely, if it’s negative, then it’s a sink. To be precise, the divergence represents the volume density of the outward fluxĀ of a vector field from an infinitesimal volume around a given point. So, in this case, it gives us the volume density of the flux of S. As you can see, the formula has exactly the same shape asĀ āˆ‡ā€¢j =Ā āˆ’āˆ‚Ļ/āˆ‚t.

So what is S? Well… Think about the more general formula for the flux out of some closed surface, which we get from integrating over the volume enclosed. It’s just Gauss’ Theorem:

Gauss Theorem

Just replace C by E, and think about what it meant: the flux of E was the field strength multiplied by the surface area, so it was the totalĀ flow of E. Likewise, SĀ represents the flow of (field) energy. Let me repeat this, because it’s an important result:

SĀ represents the flow of field energy.

Huh?Ā What flow? Per unit area? Per second? How do you define such ‘flow’? Good question. Let’s do a dimensional analysis:

  1. E is measured inĀ newton per coulomb, so [E•E] = [E2] = N2/C2.
  2. B is measured in (N/C)/(m/s). [Huh?Ā Well… Yes. I explained that a couple of times already. Just check it in my introduction to electric circuits.] So we get [B•B] = [B2] = (N2/C2)Ā·(s2/m2) but the dimension of ourĀ c2Ā factor is (m2/s2) so we’re left with N2/C2. That’s nice, because we need to add in the same units.
  3. Now we need to look at ε0. That constant usually ‘fixes’ our units, but can we trust it to do the same now? Let’s see… One of the many ways in which we can express its dimension is [ε0] =Ā C2/(NĀ·m2), so if we multiply that with N2/C2, we find that u is expressed inĀ N/m2.Ā Wow!Ā That’sĀ kindaĀ neat. Why? Well… Just multiply with m/m and its dimension becomes NĀ·m/m3Ā = J/m3, so that’s Ā joule per cubic meter, so… Yes: uĀ has got the right unit for something that’s supposed to measure energy density!
  4. OK. Now, we take the time rate of change of u, and so both the right and left of our āˆ‚u/āˆ‚t = āˆ’āˆ‡ā€¢SĀ formula are expressed in (J/m3)/s, which means that the dimension ofĀ S itself mustĀ be J/(m2Ā·s). Just check it by writing it all out: āˆ‡ā€¢SĀ = āˆ‚Sx/āˆ‚x + āˆ‚Sy/āˆ‚x + āˆ‚Sz/āˆ‚z, and so that’s something per meterĀ so, to get the dimension of S itself, we need to go from cubic meter to square meter. Done! Let me highlight the grand result:

S is the energy flow per unit area and per second.

Now we’ve got its magnitude and its dimension, but what is its direction? Indeed, we’ve been writing S as a vector, but… Well… What’s its direction indeed?

Well… Hmm… I referred you to FeynmanĀ for that derivation of that u = ε0E2/2 + ε0c2B2/2 formula energy forĀ u, and so the direction of S – I should actually say, its complete definition – comes out of that derivation as well. So… Well… I think you should just believe what I’ll be writing here for S:

S formula

So it’s the vector cross product of E and B with ε0c2Ā thrown in. It’s a simple formula really, and because I didn’t drag you through the whole argument, you should just quickly do a dimensional analysis again—just to make sure I am not talking too much nonsense. šŸ™‚ So what’s the direction? Well… You just need to apply the usual right-hand rule:

right hand rule

OK. We’re done! This S vector, which – let me repeat it – represents the energy flow per unit area and per second, is what is referred to as Poynting’s vector, and it’s a most remarkable thing, as I’ll show now. Let’s think about theĀ implicationsĀ of this thing.

Poynting’s vector in electrodynamics

The S vector is actually quite similar to the heat flow vectorĀ h, which we presented when discussing vector analysis and vector operators. The heat flow out of a surface element daĀ is the area times the component ofĀ hĀ perpendicular to da, so that’s (h•n)Ā·da = hnĀ·da. Likewise, we can writeĀ (S•n)Ā·da = SnĀ·da. The units of S and h are also the same:Ā joule per second and per square meterĀ or, using the definition of theĀ wattĀ (1 W = 1 J/s), in watt per square meter.Ā In fact, if you google a bit, you’ll find that both hĀ and S are referred to as aĀ flux density:

  1. The heat flow vector hĀ is the heat flux densityĀ vector, from which we get the heat flux through an area through the (h•n)Ā·da = hnĀ·daĀ product.
  2. The energy flow SĀ is the energy flux density vector, from which we get the energy flux through the (S•n)Ā·da = SnĀ·daĀ product.

The big difference, of course, is that we getĀ hĀ from a simpler vector equation:

h =Ā āˆ’Īŗāˆ‡T ⇔ (hx,Ā hy,Ā hz) =Ā āˆ’Īŗ(āˆ‚Tx/āˆ‚x,Ā āˆ‚Ty/āˆ‚y,āˆ‚Tz/āˆ‚x)

The vector equation for SĀ is more complicated:

S formula

So it’s a vector product. Note that S will be zero if E = 0 and/or if B = 0. So S = 0 in electrostatics, i.e. when there are no moving charges and only steady currents. Let’s examine Feynman’s examples.

The illustration below shows the geometry of theĀ E, B and SĀ vectors for a light wave. It’s neat, and totally in line with what we wrote on theĀ radiation pressure, or the momentum of light. So I’ll refer you to that post for an explanation, and to Feynman himself, of course.

light wave

OK. The situation here is rather simple. Feynman gives a few others examples that are notĀ so simple, like that ofĀ a charging capacitor, which is depicted below.

capacitor

The Poynting vector points inwards here, toward the axis. What does it mean?Ā It means the energy isn’t actually coming down the wires, but from the space surrounding the capacitor.Ā 

What?Ā I know. It’s completely counter-intuitive, at first that is. You’d think it’s the charges. But it actually makes sense. The illustration below shows how we should think of it. The charges outside of the capacitor are associated with a weak, enormously spread-out field that surrounds the capacitor. So if we bring them to the capacitor, that field gets weaker, and the field between the plates gets stronger. So the field energy which is way out moves into the space between the capacitor plates indeed, and so that’s what Poynting’s vector tells us here.

capacitor 2

Hmm… Yes. You can be skeptic. You should be. But that’s how it works. The next illustration looks at a current-carrying wire itself. Let’s first look at the B and E vectors. You’re familiar with the magnetic field around a wire, so the B vector makes sense, but what about the electric field? Aren’t wires supposed to be electrically neutral? It’s a tricky question, and we handled it in our post on the relativity of fields. The positive and negative charges in a wire should cancel out, indeed, but then it’s the negative charges that move and, because of their movement, we have the relativistic effect of length contraction, so the volumes are different, and theĀ positive andĀ negative charge density do notĀ cancel out: the wire appears to be charged, so we do have a mix of E and B! Let me quickly give you the formula: E = (2πε0)Ā·(Ī»/r), withĀ Ī» the (apparent) charge per unit length, so it’s the same formula as for a long line of charge, or for a long uniformly charged cylinder.

So we have a non-zeroĀ E and B and, hence, a non-zero Poynting vector S, whose direction isĀ radially inward, so there is a flow of energy into the wire, all around. What the hell?Ā Where does it go? Well… There’s a few possibilities here: the charges need kineticĀ energy to move, or as they increaseĀ theirĀ potentialĀ energy when moving towards the terminals of our capacitor to increase the charge on the plates or, much more mundane, the energy may be radiated out again in the form of heat. It looks crazy, but that’s how it is really. In fact, the more you think about, the more logical it all starts to sound. EnergyĀ mustĀ be conserved locally, and so it’s just field energy going in and re-appearing in some other form. So itĀ doesĀ make sense. But, yes, it’s weird, because no one bothered to teach us thisĀ in school. šŸ™‚

wire

The ‘craziest’ example is the one below: we’ve got a charge and a magnet here. All is at rest. Nothing is moving… Well… I’ll correct that in a moment. šŸ™‚ The charge (q) causes a (static) Coulomb field, while our magnet produces the usual magnetic field, whose shape we (should) recognize: it’s the usual dipole field. So E and B are not changing. But so when we calculate our Poynting vector, we see there is a circulation of S. TheĀ EƗBĀ product is notĀ zero.Ā So what’s going on here?

crazy

Well… There is no netĀ change in energy with time: the energy just circulates around and around. Everything which flows into one volume flows out again. As Feynman puts it: “It is like incompressible water flowing around.” What’s the explanation? Well… Let me copy Feynman’s explanation of this ‘craziness’:

“Perhaps it isn’t so terribly puzzling, though, when you remember that what we called a ā€œstaticā€ magnet is really a circulating permanent current. In a permanent magnet the electrons are spinning permanently inside. So maybe a circulation of the energy outside isn’t so queer after all.”

So… Well… It looks like we do need to revise some of our ‘intuitions’ here. I’ll conclude this post by quoting Feynman on it once more:

“You no doubt get the impression that the Poynting theory at least partially violates your intuition as to where energy is located in an electromagnetic field. You might believe that you must revamp all your intuitions, and, therefore have a lot of things to study here. But it seems really not necessary. You don’t need to feel that you will be in great trouble if you forget once in a while that the energy in a wire is flowing into the wire from the outside, rather than along the wire. It seems to be only rarely of value, when using the idea of energy conservation, to notice in detail what path the energy is taking. The circulation of energy around a magnet and a charge seems, in most circumstances, to be quite unimportant. It is not a vital detail, but it is clear that our ordinary intuitions are quite wrong.”

Well… That says it all, I guess. As far as I am concerned, I feel the Poyning vector makes things actuallyĀ easierĀ to understand. Indeed, the E and B vectors were quite confusing, because we had twoĀ of them, and the magnetic field is, frankly, a weirdĀ thing. Just think about the units in which we’re measuring B: (N/C)/(m/s). IĀ can’t imagine what a unit like that could possible represent, so I must assume you can’t either.Ā But so now we’ve got this Poynting vector that combines both E and B, and which represents the flow of the field energy. Frankly, I think that makes a lot of sense, and it’s surely much easier to visualize than EĀ and/or B. [Having said that, of course, you should note that E and B do have their value, obviously, if only because they represent theĀ lines of force, and so that’s something very physical too, of course.Ā I guess it’s a matter of taste, to some extent, but so I’d tend to soften Feynman’s comments on the supposed ‘craziness’ of S.

In any case… The next thing I should discuss isĀ field momentum. Indeed, if we’ve got flow, we’ve got momentum. But I’ll leave that for my next post. This topic can’t be exhausted in one post only, indeed. šŸ™‚ So let me conclude this post. I’ll do with a very nice illustration I got from the Wikipedia article on the Poynting vector. It shows the Poynting vector around a voltage source and a resistor, as well as what’s going on in-between. [Note that the magnetic field is given by the field vector H, which is related to B as follows: B = μ0(H + M), with M the magnetization of the medium. B and H are obviously just proportional in empty space, with μ0Ā as the proportionality constant.]

Poynting_vectors_of_DC_circuit

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Re-visiting relativity and four-vectors: the proper time, the tensor and the four-force

Pre-script (dated 26 June 2020): Our ideas have evolved into a full-blown realistic (or classical) interpretation of all things quantum-mechanical. In addition, I note the dark force has amused himself by removing some material. So no use to read this. Read my recent papers instead. šŸ™‚

Original post:

My previous post explained how four-vectors transformĀ from one reference frame to the other. Indeed, a four-vector isĀ notĀ just some one-dimensional array of four numbers: it represent something—a physical vector that… Well… Transforms like a vector. šŸ™‚ So whatĀ vectorsĀ are we talking about? Let’s see what we have:

  1. We knew the position four-vector already, which we’ll write as xμ = (ct, x, y, z) = (ct, x).
  2. We also proved that Aμ = (Φ,Ā Ax, Ay, Az) = (Φ,Ā A)Ā is a four-vector: it’s referred to as the four-potential.
  3. We also know the momentumĀ four-vector from theĀ LecturesĀ on special relativity. We write it as pμ = (E, px, py, pz) = (E, p), with E = γm0, p = γm0v, and γ = (1āˆ’v2/c2)āˆ’1/2Ā or, forĀ cĀ = 1, γ =Ā (1āˆ’v2)āˆ’1/2

To show that it’s notĀ just a matter of adding some fourth t-component to aĀ three-vector, Feynman gives the example of the four-velocity vector. We have vxĀ = dx/dt,Ā vyĀ = dy/dt and vzĀ = dz/dt, but a vμ = (d(ct)/dt, dx/dt, dy/dt, dz/dt) = (c, dx/dt, dy/dt, dz/dt) ‘vector’ is, obviously, not a four-vector. [Why obviously? The inner productĀ vμvμ Ā is not invariant.] In fact,Ā Feynman ‘fixes’ the problem by noting that ct, x, y and z have the ‘right behavior’, but the d/dt operator doesn’t. The d/dt operator isĀ not an invariant operator. So how does he fix it then? He tries the (1āˆ’v2/c2)āˆ’1/2Ā·d/dt operator and, yes, it turns out we do get a four-vector then. In fact, we get that four-velocity vector uμ that we were looking for:four-velocity vector[Note we assume we’re using equivalentĀ time and distance units now, soĀ cĀ = 1 andĀ v/c reduces to a new variable v.]

Now how do we know this is four-vector? How can we prove this one? It’s simple. We can get it from ourĀ pμ = (E, p) by dividing it by m0, which is an invariantĀ scalar in four dimensions too. Now, it is easy to see that a division by an invariantĀ scalar doesĀ notĀ change the transformation properties. So just write it all out, and you’ll see that pμ/m0Ā = uμ and, hence, that uμ is a four-vector too. šŸ™‚

We’ve got an interesting thing here actually: division by an invariant scalar, or applying that (1āˆ’v2/c2)āˆ’1/2Ā·d/dt operator, which is referred to as an invariant operator, on a four-vector will give us another four-vector. Why is that? Let’s switch to compatible time and distance units soĀ c = 1 so to simplify the analysis that follows.

The invariant (1āˆ’v2)āˆ’1/2Ā·d/dt operatorĀ and the proper time s

Why is theĀ (1āˆ’v2)āˆ’1/2Ā·d/dt operator invariant? Why does it ‘fix’ things? Well… Think about the invariant spacetime interval (Ī”s)2Ā = Ī”t2Ā āˆ’ Ī”x2Ā āˆ’ Ī”y2Ā āˆ’Ā Ī”z2Ā going to the limit (ds)2Ā = dt2Ā āˆ’ dx2Ā āˆ’ dy2Ā āˆ’ dz2Ā . Of course, we can and should relate this to an invariant quantity s = ∫ ds. Just like Ī”s, this quantity also ‘mixes’ time and distance. Now, we could try to associate some derivative d/ds with it because, as Feynman puts it, “it should be a nice four-dimensional operation because it is invariant with respect to a Lorentz transformation.” Yes. It should be. So let’s relate ds to dt and see what we get. That’s easy enough: dx = vxĀ·dt,Ā dy = vyĀ·dt, dz = vzĀ·dt, so we write:

(ds)2Ā = dt2Ā āˆ’ vx2Ā·dt2Ā āˆ’ vy2Ā·dt2Ā āˆ’Ā vz2Ā·dt2 ⇔ (ds)2Ā = dt2Ā·(1 āˆ’ vx2Ā āˆ’ vy2Ā āˆ’Ā vz2) = dt2Ā·(1 āˆ’ v2)

and, therefore, ds = dtĀ·(1āˆ’v2)1/2. So our operator d/ds is equal to (1āˆ’v2)āˆ’1/2Ā·d/dt, and we can apply it toĀ anyĀ four-vector, as we are sure that, as an invariant operator, it’s going to give us another four-vector. I’ll highlight the result, because it’s important:

The d/ds = (1āˆ’v2)āˆ’1/2Ā·d/dt operator is an invariant operator for four-vectors.

For example, if we apply it to xμ = (t, x, y, z), we get the very same four-velocity vector μμ:

dxμ/ds = uμ = pμ/m0

Now, if you’re somewhat awake, you should ask yourself: what is this s, really,Ā and what is this operator all about? Our new function s = ∫ ds is notĀ the distance function, as it’s got both time and distance in it. Likewise, the invariant operatorĀ d/ds = (1āˆ’v2)āˆ’1/2Ā·d/dt has both time and distance in it (the distance is implicit in the v2Ā factor). Still, it is referred to as the proper timeĀ along the path of a particle. Now why is that? If it’s got distance andĀ time in it, why don’t we call it the ‘proper distance-time’ or something?

Well… The invariant quantity s actually is the time that would be measured by a clock that’s moving along, in spacetime, with the particle. Just think of it: in the reference frame of the moving particle itself, Ī”x, Ī”yĀ and Ī”zĀ must be zero, because it’s not moving in its own reference frame. So theĀ (Ī”s)2Ā = Ī”t2Ā āˆ’ Ī”x2Ā āˆ’ Ī”y2Ā āˆ’Ā Ī”z2Ā reduces to (Ī”s)2Ā = Ī”t2, and so we’re only adding time to s. Of course, this view of things implies that theĀ proper time itself is fixed only up to some arbitrary additive constant, namely the setting of the clock at some event along the ‘world line’ of our particle, which is its path in four-dimensional spacetime. But… Well… In a way, s is the ‘genuine’ or ‘proper’ time coming with the particle’s reference frame, and so that’s why Einstein called it like that. You’ll see (later) that it plays a very important role in general relativity theory (which is a topic we haven’t discussed yet: we’ve only touched special relativity, so no gravity effects).

OK. I know this is simple and complicated at the same time: the math is (fairly) easy but, yes, it may be difficult to ‘understand’ this in some kind of intuitiveĀ way. But let’s move on.

The four-force vector fμ

We know the relativistically correct equation for the motionĀ of some charge q. It’s just Newton’s Law F = dp/dt = d(mv)/dt. The only difference is that we areĀ not assuming that m is some constant. Instead, we use the pĀ = γm0vĀ formula to get:

motion

How can we get a four-vector for the force? It turns out that we get it when applying our new invariant operator to the momentum four-vector pμ = (E, p), so we write: fμ = dpμ/ds. But pμ = m0uμ = m0dxμ/ds, so we can re-write this as fμ = d(m0·dxμ/ds)/ds, which gives us a formula which is reminiscent of the Newtonian F = ma equation:

force formula

WhatĀ isĀ this thing? Well… It’s not so difficult to verify that the x, y and z-components are just our old-fashioned Fx,Ā FyĀ andĀ Fz, so these are the components of F. The t-component is (1āˆ’v2)āˆ’1/2Ā·dE/dt. Now, dE/dt is the time rate of change of energy and, hence, it’s equal to the rate of doing work on our charge, which is equal to F•v. So we can write fμ as:

froce

The force and the tensor

We will now derive that formula which we ended the previous postĀ with. We start with calculating the spacelike components of fμ from the Lorentz formula F = q(E + vƗB). [The terminology is nice, isn’t it? The spacelike components of the four-force vector!Ā Now thatĀ sounds impressive, doesn’t it? But so… Well… It’s really just the old stuff we know already.]Ā So we start with fxĀ =Ā Fx, and write it all out:

fx

What a monster! But,Ā hey! We can ‘simplify’ this by substituting stuff by (1) the t-, x-, y- and z-components of the four-velocity vector uμ and (2) the components of our tensor Fμν = [Fij] = [āˆ‡iAjĀ āˆ’Ā āˆ‡jAi] with i, j = t, x, y, z. We’ll also pop in the diagonal FxxĀ = 0 element, just to make sure it’s all there. We get:

fx 2

Looks better, doesn’t it? šŸ™‚ Of course, it’s just the same, really. This is just an exercise in symbolism. Let me insert the electromagnetic tensor we defined in our previous post, just as a reminder of what that Fμν matrix actually is:

electromagnetic tensor final

If you read my previous post, this matrix – or the concept of a tensor – has no secrets for you. Let me briefly summarize it, because it’s an important result as well. The tensor is (a generalization of) the cross-product inĀ four-dimensional space. We take two vectors:Ā aμ =Ā (at, ax, ay, az) and bμ =Ā (bt, bx, by, bz) and then we takeĀ cross-products of their components just like we did in three-dimensional space, so we write TijĀ = aibjĀ āˆ’Ā ajbi. Now, it’s easy to see that this combination implies that TijĀ = āˆ’ TjiĀ and that TiiĀ = 0, which is why we only have sixĀ independent numbers out of the 16 possible combinations, and which is why we’ll get a so-called anti-symmetric matrix when we organize them in a matrix. In three dimensions, the very same definition of the cross-product TijĀ gives us 9 combinations, and only 3 independent numbers, which is why we represented our ‘tensor’ as a vector too! In four-dimensional space we can’t do that: six things cannot be represented by a four-vector, so weĀ need to use thisĀ matrix, which is referred to as a tensor of the second rank in four dimensions. [When you start using words like that, you’ve come a long way, really. :-)]

[…]Ā OK. Back to our four-force. It’s easy to get a similar one-liner forĀ fyĀ and fzĀ too, of course, as well as for ft. But… Yes, ft… Is it the same thing really? Let me quickly copy Feynman’s calculation for ft:

ft

ItĀ does: remember that vƗB and v are orthogonal, and so their dot product is zero indeed. So, to make a long story short, the four equations – one for each component of the four-force vector fμ – can be summarized in the following elegant equation:

motion equation

Writing this all requires a few conventions, however. For example,Ā Fμν is a 4Ɨ4 matrix and so uν has to be written as a 1Ɨ4 vector. And the formula for theĀ fxĀ and ftĀ component also make it clear that we also want to use the +āˆ’āˆ’āˆ’ signature here, so the convention for the signs in the uνFμν product is the same as that for the scalar product aμbμ. So, in short, you really need to interpret what’s being written here.

A more important question, perhaps, is: what can we do with it? Well… Feynman’s evaluation of the usefulness of this formula is rather succinct: “Although it is nice to see that the equations can be written that way, this form is not particularly useful. It’s usually more convenient to solve for particle motions by using the F = q(E + vƗB) = (1āˆ’v2)āˆ’1/2Ā·d(m0v)/dtĀ equations, and that’s what we will usually do.”

Having said that, this formula really makes good on the promise I started my previous post with: we wanted a formula, someĀ mathematical construct, that effectively presents the electromagnetic force as oneĀ force, as one physical reality. So… Well… Here it is! šŸ™‚

Well… That’s it for today. Tomorrow we’ll talk about energy and about a veryĀ mysterious concept—the electromagnetic mass. That should be fun! So I’llĀ c u tomorrow! šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Relativistic transformations of fields and the electromagnetic tensor

Pre-script (dated 26 June 2020): Our ideas have evolved into a full-blown realistic (or classical) interpretation of all things quantum-mechanical. In addition, I note the dark force has amused himself by removing some material. So no use to read this. Read my recent papers instead. šŸ™‚

Original post:

We’re going to do a very interesting piece of math here. It’s going to bring a lot of things together. The key idea is to present aĀ mathematical construct that effectively presents the electromagnetic force as oneĀ force, as one physical reality. Indeed, we’ve been saying repeatedly that electromagnetism is oneĀ phenomenon only but we’ve been writingĀ it always as something involvingĀ twoĀ vectors: he electric field vector E and the magnetic field vector B. Of course, Lorentz’ force law F = q(E + vƗB) makes it clear we’re talking one force only but… Well… There is a way of writing it all up that is much more elegant.

I have to warn you though: this post doesn’t add anything to theĀ physicsĀ we’ve seen so far: it’s all math, really and, to a large extent, math only. So if you read this blog because you’re interested in the physics only, then you may just as well skip this post. Having said that, theĀ mathematical concept we’re going to present is that of the tensorĀ and… Well… You’ll have to get to know that animal sooner or later anyway, so you may just as well give it a try right now, and see whatever you can get out of this post.

The concept of a tensor further builds on the concept of the vector, which we liked so much because it allows us to write the laws of physics as vector equations, which do notĀ change whenĀ going from one reference frame to another. In fact, we’ll see that a tensor can be described as a ‘special’ vectorĀ cross productĀ (to be precise, we’ll show that a tensor is a ‘more general’ cross product, really). So the tensor and vector concepts areĀ veryĀ closely related, but then… Well… If you think about it, the concept of a vector and the concept of a scalar are closely related, too! So we’re just moving up the value chain, so to speak: from scalar fields to vector fields to… Well… Tensor fields! And in quantum mechanics, we’ll introduce spinors, and so we also have spinor fields!Ā Having said that, don’t worry about tensor fields. Let’s first try to understand tensorsĀ tout court.Ā šŸ™‚

So… Well… Here we go.Ā Let me start with it all by reminding you of the concept of a vector, and why we like to use vectors and vector equations.

The invariance of physics and the use of vector equations

What’s a vector? You may think, naively, that any one-dimensional array of numbers is a vector. But… Well… No! In math, we may, effectively, refer to anyĀ one-dimensionalĀ array of numbersĀ as a ‘vector’, perhaps, but in physics, a vector does represent something real, something physical, and so a vector is only a vector if it transforms like a vectorĀ underĀ theĀ transformationĀ rules that apply when going from one another frame of reference, i.e. one coordinate system, to another. Examples of vectors in three dimensions are: the velocity vector v, or the momentum vector p = mĀ·v, or the position vector r.

Needless to say, the same can be said of scalars: mathematicians may define a scalar as just any real number, but it’sĀ notĀ in physics. A scalar in physics refers to something real, i.e.Ā a scalar field, like the temperature (T) inside of a block of material. In fact, think about your first vector equation: it may have been the one determining the heat flow (h), i.e. h =Ā āˆ’ĪŗĀ·āˆ‡T = (āˆ’ĪŗĀ·āˆ‚T/āˆ‚x, āˆ’ĪŗĀ·āˆ‚T/āˆ‚y, āˆ’ĪŗĀ·āˆ‚T/āˆ‚z). It immediately shows how scalar and vector fields are intimately related.

Now, when discussing the relativistic framework of physics, we introduced vectors inĀ fourĀ dimensions, i.e.Ā four-vectors.Ā The most basic four-vector is the spacetime four-vector R = (ct, x, y, z), which is often referred to as an event, but it’s just aĀ point in spacetime, really. So it’s a ‘point’ with a time as well as a spatial dimension, so it also has t in it, besides x, y and z. It is also known as the position four-vectorĀ but, again, you should think of a ‘position’ that includes time! Of course, we can re-write R as R = (ct, r), with r = (x, y, z), so here we sort of ‘break up’ the four-vector in a scalar and a three-dimensional vector, which is something we’ll do from time to time, indeed. šŸ™‚

We also have aĀ displacement four-vector, which we can write asĀ Ī”R = (cĀ·Ī”t, Ī”r). There are other four-vectors as well, including theĀ four-velocity, theĀ four-momentum and theĀ four-forceĀ four-vectors, which we’ll discuss later (in the last section of this post).

So it’s just like using three-dimensional vectors in three-dimensional physics, or ‘Newtonian’ physics, I should say: the use of four-vectors is going toĀ allow us to write the laws of physics usingĀ vector equations, butĀ in four dimensions, rather than three, so we get the ‘Einsteinian’ physics, the realĀ physics, so to speak—or the relativistically correct physics, I should say. And so these four-dimensional vector equations will also notĀ change whenĀ going from one reference frame to another, and so our four-vector will be vectors indeed, i.e. they willĀ transformĀ like a vectorĀ underĀ theĀ transformationĀ rules that apply when going from one another frame of reference, i.e. one coordinate system, to another.

What transformation? Well… In Newtonian or Galilean physics, we had translations and rotations and what have you, but what weĀ are interested in right now areĀ ‘Einsteinian’ transformations of coordinate systems, so these have to ensure that allĀ of the laws of physics that we know of, including the principle of relativity,Ā still look the same.Ā You’ve seen these transformation rules. We don’t call them the ‘Einsteinian’ transformation rules, but the LorentzĀ transformation rules, because it was a Dutch physicist (Hendrik Lorentz) who first wrote them down. So these rules are veryĀ differentĀ from the Newtonian or Galilean transformation rules which everyone assumed to be valid until the Michelson-Morley experiment unequivocally established that the speed of lightĀ did notĀ respect the Galilean transformation rules. VeryĀ different? Well… Yes. In their mathematical structure, that is. Of course, when velocities are low, i.e.Ā non-relativistic, then they yield the same result,Ā approximately, that is. However,Ā I explained that in my post on special relativity, and so I won’t dwell on that here.

Let me just jot down both sets of rules assumingĀ that the two reference frames move with respect to each other along the x- axis only, so the y- and z-component of u is zero.

Capture

The Galilean or Newtonian rules are the simple rules on the right. Going from one reference frame to another (let’s call them S and S’ respectively) is just a matter of adding or subtracting speeds: if my car goes 100 km/h, and yours goes 120 km/h, then youĀ will see my car falling behind at a speed of (minus) 20 km/h. That’s it. We could alsoĀ rotateĀ our reference frame, and our NewtonianĀ vector equationsĀ would still look the same. As Feynman notes, smilingly, it’s what a lot of armchair philosophers think relativity theory is all about, but so it’s got nothing to do with it. It’s plain wrong!

In any case, back to vectors and transformations.Ā The key to the so-calledĀ invarianceĀ of the laws of physics is the use of vectors and vector operators that transform like vectors.Ā For example, if we defined A and B as (Ax, Ay, Az) and (Bx, By, Bz), then we knew that the so-called inner productĀ A•BĀ would look the same in all rotated coordinate systems, so we can write: A•B =Ā A’•B’. So we know that if we have a product like that on both sides of an equation, we’re fine: the equation will have the same formĀ in all rotated coordinate systems. Also, the gradient, i.e. ourĀ vector operatorĀ āˆ‡Ā = (āˆ‚/āˆ‚x, āˆ‚/āˆ‚y, āˆ‚/āˆ‚z), when applied to a scalar function, gave three quantities that also transform like a vector under rotation. We also defined a vectorĀ crossĀ product, which yielded aĀ vector (as opposed to the inner product, i.e. the vectorĀ dotĀ product, which yields a scalar):

cross product

So how does this thing behave under a Galilean transformation? Well… You may or may not remember that we used this cross-product to define theĀ angular momentum L, which was a cross product of the radius vector r and the momentum vector p = mv, as illustrated below. The animation also gives the torque Ļ„, which is, loosely speaking, a measure of the turning force: it’s the cross product of r and F, i.e. the force on the lever-arm.

Torque_animation

The components of L are:

momentum angular

Now, we find that these three numbers, orĀ objectsĀ if you want, transform inĀ exactly the same wayĀ as the components of a vector.Ā However, as Feynman points out, that’s a matter of ‘luck’ really. It’s something ‘special’. Indeed,Ā you may or may not remember that we distinguished axialĀ vectors fromĀ polar vectors. L is an axial vector, while r and p are polar vectors, and so we find that, in three dimensions, the cross product of two polar vectors will always yields an axial vector. Axial vectors are sometimes referred to asĀ pseudovectors, which suggests that they are ‘not so real’ as… Well… Polar vectors, which are sometimes referred to as ‘true’ vectors. However, it doesn’t matter when doing these Newtonian or Galilean transformations: pseudo or true, both vectors transform like vectors. šŸ™‚

But so… Well… We’re actually getting a bit of a heads-up here: if we’d be mixing (or ‘crossing’) polar and axial vectors, or mixing axial vectors only, so if we’d define something involvingĀ LĀ andĀ pĀ (rather than r and p), or something involvingĀ LĀ andĀ Ļ„, then we may notĀ be so lucky, and then we’d have to carefully examine our cross-product, or whatever other product we’d want to define, because its components mayĀ notĀ behave like a vector.

Huh? Whatever other product we’d want to define? Why are you saying that?Ā Well…Ā We actuallyĀ can think of other products. For example, if we haveĀ two vectors a = (ax, ay,Ā az) and b = (bx, by, bz), then we’ll haveĀ nine possible combinations of their components, which we can write as TijĀ = aibj. So that’s like Lxy, LyzĀ and LzxĀ really. Now, you’ll say: “No. It isn’t. We don’t have nine combinations here. Just three numbers.” Well… Think about it: we actually doĀ haveĀ nineĀ LijĀ combinations too here, as we can write: LijĀ = riĀ·pj – rjĀ·pi. It just happens that, with this definition, only threeĀ of these combinations LijĀ are independent. That’s because the other six numbers are either zero or the opposite. Indeed, it’s easy to verify thatĀ LijĀ = –LjiĀ , and LiiĀ  = 0. So… Well… It turns out that the three components of our LĀ = rƗp ‘vector’ are actually a subset of a set of nineĀ LijĀ numbers.Ā So… Well… Think about it. We cannot just do whatever we want with our ‘vectors’. We need to watch out.

In fact, I do not want to get too much ahead of myself, but I can already tell you that the matrix with these nineĀ TijĀ = aibjĀ combinations is what is referred to as the tensor. To be precise, it’s referred to as a tensor of the second rank in three dimensions. The ‘second rank’, aka as ‘degree’ or ‘order’ refers to the fact that we’ve got two indices, and the ‘three dimensions’ is because we’re using three-dimensional vectors. We’ll soon see that the electromagnetic tensor is also of the second rank, but it’s a tensor in four dimensions. In any case, I should not get ahead of myself. Just note what I am saying here: the tensor is like a ‘new’ product of two vectors, a new type of ‘cross’ product really (because we’re mixing the components, so to say), but it doesn’t yield a vector: it yields aĀ matrix. For three-dimensional vectors, we get a 3Ɨ3 matrix. For four-vectors, we’ll get a 4Ɨ4 matrix. And so the full truth about our angular momentum vector L, is the following:

  1. There is a thing which we call the angular momentum tensor. It’s a 3Ɨ3 matrix, so it has nine elements which are defined as: LijĀ = riĀ·pj – rjĀ·pi. BecauseĀ of this definition, it’s an antisymmetric tensor of the second order in three dimensions, so it’s got only three independentĀ components.
  2. The three independent elements are the components of our ‘vector’ L, and picking them out and calling these three components a ‘vector’ is actually a ‘trick’ that only works in three dimensions. They really just happen toĀ transform like a vector under rotation or under whatever Galilean transformation! [By the way, do you know understand why I was saying that we can look at a tensor as a ā€˜more general’ cross product?]
  3. In fact, in four dimensions, we’ll use a similar definition and define 16 elementsĀ FijĀ as FijĀ = āˆ‡iAjĀ āˆ’Ā āˆ‡jAi, using the two four-vectors āˆ‡Ī¼Ā and Aμ (so we have 4Ɨ4 = 16 combinations indeed), out of whichĀ only sixĀ will be independent for the very same reason: we have an antisymmetric vector combination here, FijĀ = āˆ’FjiĀ and FiiĀ = 0. šŸ™‚ However, because we cannotĀ represent six independent things by four things, we doĀ notĀ get some other four-vector, and so that’s why we cannot apply the same ‘trick’ in four dimensions.

However, here I amĀ getting way ahead of myself and so… Well… Yes. Back to the main story line. šŸ™‚ So let’s try to move to the next level of understanding, which is… Well…

Because of guys like Maxwell and Einstein, we now knowĀ that rotations are part of the Newtonian world, in which time and space are neatly separated, and that things are notĀ so simple in Einstein’s world, which is the real world, as far as we know, at least! Under a Lorentz transformation, the new ā€˜primed’ space and time coordinates are a mixture of the ā€˜unprimed’ ones. Indeed, the new x’Ā is a mixture of x and t, and the new t’Ā is a mixture of x and t as well. [Yes, please scroll all the way up and have a look at the transformation on the left-hand side!]

So youĀ don’t have that under a Galilean transformation: in the Newtonian world, space and time are neatly separated, and time is absolute, i.e. it is the same regardless of the reference frame. In Einstein’s world – our world – that’s not the case: time is relative, orĀ localĀ as Hendrik Lorentz termed it quite appropriately,Ā and so it’s space-time – i.e. ā€˜some kind of union of space and time’ as Minkowski termed it – that transforms.

So that’s why physicists useĀ four-vectorsĀ toĀ keep track of things. These four-vectors always have three space-like components, but they also include one so-calledĀ time-like component.Ā It’s the only way to ensure thatĀ the laws of physics are unchanged when moving with uniform velocity.Ā Indeed, any true law of physics we write down must be arranged so that the invariance of physics (as a “fact of Nature”, as Feynman puts it) is built in, and so that’s why we use Lorentz transformations and four-vectors.

In the mentioned post, I gave a few examples illustrating how the Lorentz rules work. Suppose we’re looking at some spaceship that is moving at half the speed of light (i.e. 0.5c) and that, inside the spaceship, some object is also moving at half the speed of light, as measured in the reference frame of the spaceship, then we get the rather remarkable result that, from ourĀ point of view (i.e. ourĀ reference frame as observer on the ground), that object is notĀ going as fast as light, as Newton or Galileo – and most present-day armchair philosophers šŸ™‚ – would predict (0.5cĀ +Ā 0.5cĀ = c). We’d see it move at a speed equal to vĀ =Ā 0.8c. Huh?Ā How do we know that? Well… We can derive a velocity formula from the Lorentz rules:

Capture

So now you can just put in the numbers now:Ā vxĀ = (0.5c + 0.5c)/(1 + 0.5Ā·0.5) = 0.8c. See?

Let’s do another example. Suppose we’re looking at a light beam inside the spaceship, so something that’s traveling at speed c itself in the spaceship. How does that look to us? The Galilean transformation rules say its speed should be 1.5c, but that can’t be true of course, and the Lorentz rules save us once more: vxĀ = (0.5cĀ + c)/(1 + 0.5Ā·1) = c, so it turns out that the speed of light doesĀ notĀ depend on the reference frame: it looks the same – both to the man in the ship as well as to the man on the ground. As Feynman puts it: “This is good, for it is, in fact, what the Einstein theory of relativity was designed to do in the first place—so it hadĀ betterĀ work!” šŸ™‚

So let’s now apply relativity to electromagnetism. Indeed, that’s what this post is all about! However, before I do so, let me re-write the Lorentz transformation rules forĀ cĀ = 1. We can equate the speed of light to one, indeed, when measure time and distance in equivalent units. It’s just a matter of ditching our seconds for meters (so our time unit becomes the time that light needs to travel a distance of one meter), or ditching our meters for seconds (so our distance unit becomes the distance that light travels in one second). You should be familiar with this procedure. If not, well… Check out my posts on relativity. So here’s the same set of rules for cĀ = 1:

Lorentz rules

They’re much easier to remember and work with, and so that’s good, because now we need toĀ look at how these rules work with four-vectors and the various operations and operators we’ll be defining on them. Let’s look at that step by step.

Electrodynamics in relativistic notation

Let me copy the UniversalĀ Set of Equations and Their Solution once more:

frame

The solution for Maxwell’s equations is given in terms of the (electric) potential Φ and the (magnetic) vectorĀ potential A. I explained that in my post on this, so I won’t repeat myself too much here either. The only point you should note is that this solution is the result of a special choice of Φ andĀ A, which we referred to as the Lorentz gauge.Ā We’ll touch upon this condition once more, so just make a mental note of it.

Now, E and B do not correspond to four-vectors: theyĀ dependĀ on x, y, z and t, but they haveĀ threeĀ components only:Ā Ex, Ey,Ā Ez, and Bx, By, and BzĀ respectively. So we have sixĀ independent terms here, rather thanĀ four things that, somehow, we could combine into some four-vector. [Does this ring a bell? It should. :-)] Having said that, it turns out that weĀ canĀ combine Φ andĀ AĀ into a four-vector, which we’ll refer to as the four-potentialĀ and which we’llĀ will write as:

Aμ = (Φ, A) = (Φ, Ax, Ay, Az) = (At, Ax, Ay, Az) with At = Φ.

So that’s a four-vector just likeĀ R = (ct, x, y, z).

How do we know that Aμ is a four-vector? Well… Here I need to say a few things about those Lorentz transformation rules and, more importantly, about the required condition ofĀ invarianceĀ under a Lorentz transformation. So, yes, here we need to dive into the math.

Four-vectors and invariance under Lorentz transformations

When you were in high-school, you learned how toĀ rotateĀ your coordinate frame. You also learned that the distance of a point from the origin does not change under a rotation, so you’d writeĀ r’2Ā = x’2Ā + y’2Ā + z’2Ā =Ā r2Ā =Ā x2Ā + y2Ā + z2, and you’d say that r2Ā is an invariant quantity under a rotation.Ā Indeed, transformations leave certain things unchanged. From the Lorentz transformation rules itself, it is easy to see that

cĀ·t’2 – x’2 – y’2 –z ‘2 = cĀ·t2 –x2 – y2Ā  – z2, or,

if cĀ = 1, thatĀ t’2 – x’2 – y’2 – z’2 = t2 – x2 – y2Ā  – z2,

is anĀ invariantĀ under a Lorentz transformation. We found the same for the so-calledĀ spacetimeĀ interval Ī”s2Ā  =Ā Ī”r2 – cĪ”t2, which we write as Ī”s2Ā  =Ā Ī”r2 – Ī”t2Ā as we chose our time or distance units such that cĀ = 1. [Note that, from now on, we’ll assume that’s the case, so cĀ = 1 everywhere. We can always change back to our old units when we’re done with the analysis.] Indeed, such invariance allowed us to define spacelike,Ā timelikeĀ and lightlikeĀ intervals using the so-called light cone emanating from a single event and traveling in all directions.

You should note that, for four-vectors, we do not have a simple sum of three terms. Indeed, we don’t write x2Ā + y2Ā + z2Ā but t2 – x2 – y2Ā  – z2. So we’ve got a +āˆ’āˆ’āˆ’ thing here or, it’s just another convention, we could also work with a āˆ’+++ sum of terms. The convention is referred to as the signature, and we will use the so-calledĀ metric signature here, which is +āˆ’āˆ’āˆ’. Let’s continue the story.Ā Now, all four-vectors aμ = (at, ax, ay, az) have this property that:

at‘2 – ax‘2 – ay‘2 – az‘2 = at2 – ax2 – ay2Ā  – az2.

[The primed quantities are, obviously, the quantities as measured in the other reference frame.]Ā So. Well… Yes. šŸ™‚ But… Well… Hmm… We can sayĀ that our four-potential vector is a four-vector, butĀ so we still have toĀ proveĀ that. So we need to prove that Φ’2 – Ax‘2 – Ay‘2 – Az‘2 = Φ2 – Ax2 – Ay2Ā  – Az2Ā for ourĀ four-potential vectorĀ Aμ = (Φ, A). So… Yes… How can we do that? The proof isĀ notĀ so easy, but you need to go through it as it will introduce some more concepts and ideas you need to understand.

In my post on the Lorentz gauge, I mentioned that Maxwell’s equations can be re-written in terms of Φ andĀ A, rather than in terms of E and B. The equations are:

Equations 2

The expression look rather formidable, but don’t panic: just look at it. Of course, you need to be familiar with the operators that are being used here, so that’s the Laplacian āˆ‡2Ā and the divergence operator āˆ‡ā€¢ that’s being applied to the scalar Φ and the vector A. I can’t re-explain this. I am sorry. Just check my posts on vector analysis.Ā You should also look at the third equation: that’s just the Lorentz gauge condition, which we introduced when derivingĀ these equations from Maxwell’s equations. Having said that, it’s the first and second equation which describe Φ and A as a function of the charges and currents in space, and so that’s what matters here. So let’s unfold the first equation. It says the following:

potential formula

In fact, if we’d be talkingĀ freeĀ or empty space, i.e. regions where there are no charges and currents, then the right-hand side would be zero and this equation would then represent a wave equation, so some potential Φ that is changing in time and moving out at the speed c. Here again, I am sorry I can’t write about this here: you’ll need to check one of my posts on wave equations. If you don’t want to do that, you should believe me when I say that, if you see an equation like this:

f8then the functionĀ ĪØ(x, t) must be some function

solution

Now, that’s a function representing a wave traveling at speed c, i.e. the phase velocity. Always? Yes.Ā Always! It’s got to do with the x āˆ’ ct and/or x +Ā ctĀ  argument in the function. But, sorry, I need to move on here.

The unfolding of the equation with Φ makes it clear that we have four equations really. Indeed, the second equation is three equations: one for Ax, one forĀ Ay, and one forĀ AzĀ respectively. The four quantities on the right-hand side of these equations are ρ, jx, jyĀ and jzĀ respectively, divided by ε0, which is a universal constant which does notĀ change when going from one coordinate system to another.Ā Now, the quantities ρ, jx, jyĀ and jzĀ transform like a four-vector. How do we know that? It’s just the charge conservation law. We used it when solving the problem of the fields around a moving wire, when we demonstrated theĀ relativityĀ of the electric and magnetic field. Indeed, the relevant equations were:

Lorentz j and rho

You can check that against the Lorentz transformation rules forĀ cĀ = 1. They’re exactly the same, but so we chose t = 0, so the rules are even simpler. Hence, the (ρ,Ā jx, jy, jz) vector is, effectively, aĀ four-vector, and we’ll denote it by jμ = (ρ, j).Ā I nowĀ need to explain something else. [And, yes,Ā I know this is becoming a veryĀ long story but… Well… That’s how it is.]

It’s about our operatorsĀ āˆ‡, āˆ‡ā€¢, āˆ‡Ć— and āˆ‡2Ā , so that’s the gradient, theĀ divergence, curlĀ and LaplacianĀ operator respectively: they all have a four-dimensional equivalent. Of course, that won’t surprise you. 😦 Let me just jot all of them down, so we’re done with that, and then I’ll focus on the four-dimensional equivalent of the LaplacianĀ Ā āˆ‡ā€¢āˆ‡ =Ā āˆ‡2Ā , which is referred to as theĀ D’Alembertian, and which is denoted byĀ ā–”2, because that’s the one we need to prove that our four-potential vector is a realĀ four-vector. [I know: ā–”2Ā is a tiny symbol for a pretty monstrous thing, but I can’t help it: my editor tool is pretty limited.]

Four-vectors

Now, we’re almost there. Just hang in for a little longer. It should be obvious that we can re-write those two equations with Φ, A, ρ and j, as:

Formula d'alembertian 2

Just to make sure, let me remind you that Aμ = (Φ, A) and thatĀ jμ = (ρ, j). Now, our new D’Alembertian operator is just an operator—a prettyĀ formidableĀ operator but, still, it’s an operator, and so itĀ doesn’t change when the coordinate system changes, so the conclusion is that,Ā IFĀ jμ = (ρ, j) is a four-vector – which it is – and, therefore, transforms like a four-vector,Ā THENĀ the quantities Φ, Ax, Ay, and AzĀ must also transformĀ like a four-vector, which means they areĀ (the components of) a four-vector.

So… Well… Think about it, but not too long, because it’s just an intermediate result we had to prove. So that’s done. But we’re not done here. It’s just the beginning, actually. :-/ Let me repeat our intermediate result:

Aμ = (Φ, A) is a four-vector. We call it the four-potential vector.

OK. Let’s continue. Let me firstĀ draw your attention to that expression with the D’Alembertian above. Which expression? This one:

Formula d'alembertian 2

What about it? Well… You should note thatĀ the physics of that equation is just the same as Maxwell’s equations. So it’s one equation only, but it’s got it all.

It’s quite a pleasure to re-write it in such elegant form. Why? Think about it: it’s a four-vector equation: we’ve got a four-vector on the left-hand side, and a four-vector on the right-hand side. Therefore, this equation is invariant under a transformation. So, therefore,Ā it directly shows the invariance of electrodynamics under the Lorentz transformation.

Huh? Yes. You may think about this a little longer. šŸ™‚

To wrap this up, I should also note that we can also express the gauge condition using our new four-vector notation. Indeed, we can write it as:

Lorentz condition

It’s referred to as the Lorentz condition and it is, effectively, a condition for invariance, i.e. it ensures that the four-vector equation above does stay in the form it is in for all reference frames. Note that we’re re-writing it using the four-dimensional equivalent of the divergence operatorĀ āˆ‡ā€¢, but so we don’t have a dot between āˆ‡Ī¼Ā and Aμ. In fact, the notation is pretty confusing, and it’s easy to think we’re talking some gradient, rather than the divergence. So let me therefore highlight the meaning of both once again. It looks the same, but it’s two veryĀ different things: the gradient operates on a scalar, while the divergence operates on a (four-)vector. Also note the +āˆ’āˆ’āˆ’ signature is only there for theĀ gradient, not for the divergence!

example

You’ll wonder why they didn’t use some • orĀ āˆ— symbol, and the answer: I don’t know. I know it’s hard to keep inventing symbols for all these different ‘products’ – the āŠ— symbol, for example, is reserved forĀ tensorĀ products, which we won’t get into – but… Well… I think they could have done something here. 😦

In any case… Let’s move on. Before we do, please note that we can also re-write our conservation law for electric charge using our new four-vector notation. Indeed, you’ll remember that we wrote that conservation law as:

conservation law

Using our new four-vector operator āˆ‡Ī¼, we can re-write that as āˆ‡Ī¼jμ = 0. So all of electrodynamics can be summarized in the two equations only—Maxwell’s law and the charge conservation law:

all

OK. We’re now ready to discuss the electromagnetic tensor. [I know… This is becoming an incredibly long and incredibly complicated piece but, ifĀ you get through it, you’ll admitĀ it’s really worth it.]

The electromagnetic tensor

The whole analysis above was done in terms of the Φ and A potentials. It’s time to get back to our field vectorsĀ E and B. We know we can easily get them from Φ and A, using the rules we mentioned as solutions:

E and B solutions

These two equations shouldĀ notĀ look as yet another formula. They are essential, and you should be able to jot them down anytime anywhere. They should be on your kitchen door, in your toilet and above your bed. šŸ™‚Ā For example, the second equation gives us theĀ components of the magnetic field vector B:

B field components

Now, look at these equations. The x-component is equal to a couple of terms that involve only y– and z-components. The y-component is equal to something involving only xĀ and z.Ā Finally, the z-component only involves x and y. Interesting. Let’s define a ‘thing’ we’ll denote by FzyĀ and define as:

F definition

So now we can write: BxĀ = Fzy,Ā ByĀ = Fxz, andĀ BzĀ = Fxy. Now look at our equation for E. It turns out the components of E are equal to things likeĀ Fxt, FytĀ and Fzt! Indeed,Ā FxtĀ =Ā āˆ‚Ax/āˆ‚tĀ āˆ’Ā āˆ‚At/āˆ‚x = Ex!

But… Well… No. 😦 The sign is wrong!Ā ExĀ = āˆ’āˆ‚Ax/āˆ‚tāˆ’āˆ‚At/āˆ‚x, so we need to modify our definition of Fxt. When the t-component is involved, we’ll define our ‘F-things’ as:

time f

So we’ve got a plus instead of a minus. It looks quite arbitrary but, frankly, you’ll have to admit it’s sort of consistent with our +āˆ’āˆ’āˆ’ signatureĀ for our four-vectors and, in just a minute, you’ll see it’s fully consistent with our definition of the four-dimensional vector operatorĀ āˆ‡Ī¼Ā = (āˆ‚/āˆ‚t, āˆ’āˆ‚/āˆ‚x,Ā āˆ’āˆ‚/āˆ‚y, āˆ’āˆ‚/āˆ‚z). So… Well… Let’s go along with it.

What about the Fxx, Fyy, FzzĀ and FttĀ terms? Well…Ā FxxĀ =Ā āˆ‚Ax/āˆ‚x āˆ’Ā āˆ‚Ax/āˆ‚x = 0, and it’s easy to see that FyyĀ and FzzĀ are zero too. ButĀ Ftt? Well… It’s a bit tricky but, applying our definitions carefully, we see that FttĀ must be zero too. In any case, theĀ FttĀ = 0 will become obvious as we will be arranging these ‘F-things’ in a matrix, which is what we’ll do now.Ā [Again: does this ring a bell? If not, it should. :-)]

Indeed, we’ve got sixteen possible combinations here, which Feynman denotes as Fμν, which is somewhat confusing, because Fμν usually denotes theĀ 4Ɨ4 matrixĀ representing all of these combinations. So let me use the subscripts i and j instead, and define FijĀ as:

FijĀ =Ā āˆ‡iAjĀ āˆ’Ā āˆ‡jAi

with āˆ‡iĀ being the t-, x-, y- orĀ z-component of āˆ‡Ī¼Ā =Ā (āˆ‚/āˆ‚t, āˆ’āˆ‚/āˆ‚x,Ā āˆ’āˆ‚/āˆ‚y,Ā āˆ’āˆ‚/āˆ‚z) and, likewise, AiĀ being the t-, x-, y- orĀ z-component of Aμ =Ā (Φ, Ax,Ā Ay,Ā Az). Just check it: FzyĀ = āˆ’āˆ‚Ay/āˆ‚z +Ā āˆ‚Az/āˆ‚y = āˆ‚Az/āˆ‚y āˆ’ āˆ‚Ay/āˆ‚z = Bx, for example, andĀ FxtĀ =Ā āˆ’āˆ‚Ī¦/āˆ‚x āˆ’Ā āˆ‚Ax/āˆ‚tĀ = Ex. So theĀ +āˆ’āˆ’āˆ’ conventionĀ works. [Also note that it’s easier now to see that FttĀ = āˆ‚Ī¦/āˆ‚t āˆ’ āˆ‚Ī¦/āˆ‚t = 0.]

We can now arrange the FijĀ in a matrix. This matrix is antisymmetric, because FijĀ = – Fji, and its diagonal elements are zero. [For those of you who love math: note that the diagonal elements of an antisymmetric matrix are always zero because of the FijĀ = – FjiĀ constraint: just use k = i = j in the constraint.]

Now that matrix is referred to as the electromagnetic tensor and it’s depicted below (we pluggedĀ cĀ back in, remember thatĀ B’s magnitude is 1/c times E’s magnitude).

electromagnetic tensor final

So… Well… Great ! We’re done! Well… Not quite. šŸ™‚

We can get this matrix in a number of ways. The least complicated way is, of course, just to calculate all FijĀ components and them put them in a [Fij] matrix using theĀ iĀ as the row number and theĀ jĀ as the column number. You need to watch out with the conventions though, and soĀ i and j startĀ onĀ t and end on z. šŸ™‚

The other way to do it is to write theĀ āˆ‡Ī¼Ā = (āˆ‚/āˆ‚t, āˆ’āˆ‚/āˆ‚x,Ā āˆ’āˆ‚/āˆ‚y,Ā āˆ’āˆ‚/āˆ‚z) operator as a 4Ɨ1 column vector, which you then multiply with the four-vector Aμ written as a 4Ɨ1 row vector. So āˆ‡Ī¼Aμ is then aĀ 4Ɨ4 matrix, which we combine with its transpose, i.e.Ā (āˆ‡Ī¼Aμ)T, as shown below. So what’s written below is (āˆ‡Ī¼Aμ) āˆ’ (āˆ‡Ī¼Aμ)T.

matrix

If you google, you’ll see there’s more than one way to go about it, so I’d recommend you just go through the motions and double-check the whole thing yourself—and please do let me know if you find any mistake! In fact, the Wikipedia article on the electromagnetic tensor denotes the matrix above asĀ Fμν, rather than asĀ Fμν, which is the sameĀ tensorĀ but in its so-calledĀ covariantĀ form, but so I’ll refer you to that article as I don’t want to make things even more complicated here! As said, there’s differentĀ conventionsĀ around here, and so you need to double-check what is what really. šŸ™‚

Where are we heading with all of this? The next thing is to look at theĀ LorentzĀ transformation of theseĀ FijĀ =Ā āˆ‡iAjĀ āˆ’Ā āˆ‡jAiĀ components, because then we know how our E and B fields transform. Before we do so, however, we should note the more general results and definitions which we obtained here:

1. The Fμν matrix (a matrix is just a multi-dimensional array, of course) is a so-called tensor. It’s a tensor of the second rank, because it has two indices in it. We think of it as a very special ‘product’ of two vectors, not unlike the vector cross product aĀ Ć— b, whose components were also defined by a similar combination of the components of a and b. Indeed, we wrote:

cross product

So one should think of a tensor as “another kind of cross product” or, preferably, and as Feynman puts it, as a “generalization of the cross product”.

2.Ā In this case, the four-vectors are āˆ‡Ī¼Ā =Ā (āˆ‚/āˆ‚t, āˆ’āˆ‚/āˆ‚x,Ā āˆ’āˆ‚/āˆ‚y,Ā āˆ’āˆ‚/āˆ‚z) and Aμ =Ā (Φ, Ax,Ā Ay,Ā Az). Now, you will probably say that āˆ‡Ī¼Ā is an operator, not a vector, and you are right. However, we know that āˆ‡Ī¼Ā behaves like a vector, and so this is just a special case. The point is: because the tensor is based on four-vectors, the Fμν tensor is referred to as a tensor of the second rank in four dimensions. In addition, because of the FijĀ = – FjiĀ result, Fμν is an asymmetric tensor of the second rank in four dimensions.

3.Ā Now, the whole point is to examine how tensors transform. We know that the vector dot product, aka the inner product, remains invariantĀ under a Lorentz transformation, both in three as well as in four dimensions, but what about the vector cross product, and what about the tensor? That’s what we’ll be looking at now.

The Lorentz transformation of the electric and magnetic fields

Cross products are complicated, and tensors will be complicated too. Let’s recall our example in three dimensions, i.e. the angular momentum vectorĀ L, which was a cross product of the radius vector r and the momentum vector p = mv, as illustrated below (the animation also gives the torque Ļ„, which is, loosely speaking, a measure of the turning force).

Torque_animation

The components of L are:

momentum angular

Now, this particular definition ensures that LijĀ turns out to be an antisymmetric object:

three-vector

So it’s a similar situation here. We have nineĀ possible combinations, but only threeĀ independent numbers. So it’s a bit like our tensor in four dimensions: 16 combinations, but only 6 independent numbers.

Now, it so happens that that these three numbers, orĀ objectsĀ if you want, transform inĀ exactly the same wayĀ as the components of a vector.Ā However, as Feynman points out, that’s a matter of ‘luck’ really. In fact, Feynman points out that, when we have two vectors a = (ax, ay,Ā az) and b = (bx, by, bz), we’ll haveĀ nineĀ products TijĀ = aibjĀ which will also form aĀ tensorĀ of the second rank (cf. the two indices) but which, in general, will not obey the transformation rules we got for theĀ angular momentumĀ tensor, whichĀ happenedĀ to be an antisymmetric tensor of the second rank in three dimensions.

To make a long story short, it’s not simple in general, and surely not here: with E and B, we’ve gotĀ sixĀ independent terms, and so we cannotĀ represent six things by four things, so the transformation rules for E and B will differ from those for a four-vector. So what areĀ they then?

Well… Feynman first works out the rules for the general antisymmetric vector combination GijĀ = aibjĀ āˆ’ ajbi, withĀ aiĀ and bjĀ the t-, x-, y- or z-component of the four-vectors aμ = (at, ax, ay, az) and bμ = (bt, bx, by, bz) respectively. The idea is to first get some general rules, and then replace GijĀ = aibjĀ āˆ’ ajbiĀ by FijĀ =Ā āˆ‡iAjĀ āˆ’Ā āˆ‡jAi, of course! So let’s apply the Lorentz rules, which – let me remind you – are the following ones:

Lorentz rules

So we get:

set 1

The rest is all very tedious: you just need to plug these things into the variousĀ GijĀ = aibjĀ āˆ’ ajbiĀ formulas. For example, for G’tx, we get:

G1

Hey! That’s justĀ G’tx, so we find that G’txĀ =Ā Gtx! What about the rest? Well… ThatĀ yields something different. Let me shorten the story by simply copying Feynman here:

resulsts

So… Done!

So what?

Well… Now we just substitute. In fact, thereĀ areĀ two alternative formulations of the Lorentz transformations of E and B. They are given below (note the units are such thatĀ c = 1):

result 1 result 2

In addition, there is a third equivalent formulation which is more practical, and also simpler, even if it puts theĀ c‘s back in. It re-defines the field components, distinguishing only two:

  1. The ‘parallel’ components E||Ā and B||Ā along theĀ x-direction ( because they are parallel to the relative velocity of the S and S’ reference frames), and
  2. The ‘perpendicular’ or ‘total transverse’ componentsĀ E⊄ and B⊄, which are the vector sums of the y- and z-components.

So that gives us four equations only:

result 3

And, yes, we areĀ done now. This is the Lorentz transformation of the fields. I am sure it has left you totally exhausted. Well… If not… […] It sure left me totally exhausted. šŸ™‚

To lighten things up, let me insert an image of how the transformed field E actually looks like. The first image is the reference frame of a charge itself: we have a simple Coulomb field. The second image shows the charge flying by. Its electric field is ‘squashed up’. To be precise, it’s just like the scale ofĀ xĀ is squashed up by a factorĀ ((1āˆ’v2/c2)1/2. Let me refer you to Feynman for the detail of the calculations here.

field

OK. So that’s it. You may wonder: what about that promise I made? Indeed, when I started this post, I said I’dĀ present aĀ mathematical construct that presents the electromagnetic force as oneĀ force only, as one physical reality, but so we’re back writing all of it in terms of twoĀ vectors—the electric field vector E and the magnetic field vector B. Well… What can I say? IĀ didĀ present the mathematical construct: it’s the electromagnetic tensor. So it’s that antisymmetric matrix really, which one can combine with aĀ transformation matrixĀ embodying the Lorentz transformation rules. So, IĀ didĀ what I promised to do. But you’re right: IĀ amĀ re-presenting stuff in the old style once again.

The second objection that you may have—in fact, that youĀ shouldĀ have, is that all of this has been rather tedious. And you’re right.Ā The whole thing just re-emphasizes the value of using the four-potential vector. It’s obviouslyĀ muchĀ easier to takeĀ thatĀ vector from one reference frame to another – so we just apply the Lorentz transformation rules to Aμ = (Φ, A) and get Aμ‘ = (Φ’, A’) from it – and then calculate E’ and B’ from it, rather than trying to remember those equations above.Ā However, that’s not the point, or…

Well… It is and it isn’t. We wanted to get away from thoseĀ twoĀ vectors E and B, and show thatĀ electromagnetism is reallyĀ oneĀ phenomenon only, and so that’s where the concept of the electromagnetic tensor came in. There were two objectives here: the first objective was to introduce you to the concept of tensors, which we’ll need in the future. The second objective was to show you that, while Lorentz’ force law – F = q(E + vƗB) makes it clear we’re talking one force only, there is a way of writing it all up that is much more elegant.

I’ve introduced the concept of tensors here, so the first objective should have been achieved. As for the second objective, I’ll discuss that in my next post, in which I’ll introduce the four-velocity vector μμ as well as the four-force vectorĀ fμ. It will explain the following beautiful equation of motion:

motion equation

NowĀ thatĀ looks very elegant and unified, doesn’t it? šŸ™‚

[…] Hmm… No reaction. I know… You’re tired now, and you’re thinking: yet another way of representing the same thing? Well… Yes! So…

OK… Enough for today. Let’s follow up tomorrow.

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Electric circuits (1): the circuit elements

OK. No escape. It’s part of physics. I am not going to go into the nitty-gritty of it all (because this is a blog about physics, not about engineering)Ā but it’s good to review the basics, which are, essentially, Kirchoff’s rules. Just for the record, GustavĀ Kirchhoff was a German genius who formulated these circuit laws while he was still a student, when he was like 20 years old or so. He did it as aĀ seminar exerciseĀ 170 years ago, and then turned it into doctoral dissertation. Makes me think of that Dire Straits song—That’s the way you do it—Them guys ain’t dumb. šŸ™‚

So this post is, in essence, just an ‘explanation’ of Feynman’s presentation of Kirchoff’s rules, so I am writing this post basically for myself, so as to ensure I am not missing anything. To be frank, Feynman’s use of notation when working with complex numbers is confusing at times and so, yes, I’ll do some ‘re-writing’ here.Ā The nice thing about Feynman’s presentation of electrical circuits is that he sticks to Maxwell’s Laws when describing all ideal circuit elements, so he keeps using line integrals of the electric field EĀ around closed paths (that’s what a circuit is, indeed) to describe the so-calledĀ passive circuit elements, and he also recapitulates the idea of theĀ electromotive forceĀ when discussing the so-calledĀ activeĀ circuit element, so that’s the generator. That’s nice, because it links it all with what we’ve learned so far, i.e. theĀ fundamentalsĀ as expressed in Maxwell’s set of equations. Having said that, I won’t make that link here in this post, because I feel it makes the whole approach rather heavy.

OK. Let’s go for it. Let’s first recall the concept ofĀ impedance.

The impedance concept

There are three idealĀ (passive) circuit elements: the resistor, the capacitor and the inductor. RealĀ circuit elements usually combine characteristics of all of them, even if they are designed to work like ideal circuit elements. Collectively, these ideal (passive) circuit elements are referred to as impedances, because… Well… Because they have someĀ impedance. In fact, you should note that, if we reserve the terms ending with -ance for theĀ propertyĀ of the circuit elements, and those ending on -or for the objects themselves, then we should call them impedors. However, that term does not seem to have caught on.

You already know what impedance is. I explained it before, notably in my post on the intricacies related to self- and mutual inductance. Impedance basically extends the concept ofĀ resistance, as we know it fromĀ direct current (DC)Ā circuits, toĀ alternating currentĀ (AC) circuits. To put it simply, when AC currents are involved – so when the flow of charge periodically changes reverses direction – then it’s likely that, because of the properties of the circuit, the current signal will lag the voltage signal, and so we’ll have some phase differenceĀ telling us by how much. So, resistance is just a simple realĀ number R – it’sĀ the ratioĀ between (1) the voltage that is being applied across the resistor and (2) the current through it, so we write R = V/I – and it’s got aĀ magnitudeĀ only, butĀ impedance isĀ a ‘number’ that has both a magnitude as well as phase, so it’s aĀ complexĀ number, or a vector.

In engineering, such ‘numbers’ with a magnitude as well as a phase are referred to as phasors. A phasor represents voltages, currents and impedances as a phase vector (note the boldĀ italics: they explain how we got the pha-sorĀ term). It’s just a rotatingĀ vector really.Ā So a phasor has a varying magnitude (A) and phase (φ) , which is determined by (1) some maximum magnitude A0, (2) some angular frequency ω and (3) some initial phaseĀ (Īø). So we can write the amplitudeĀ A as:

A = A(φ) = A0Ā·cos(φ) =Ā A0Ā·cos(ωt + Īø)

As usual, Wikipedia has a nice animation for it:

Unfasor

In case you wonder why I am using aĀ cosineĀ rather than aĀ sineĀ function, the answer is that it doesn’t matter: the sine and the cosine are the same function except for a Ļ€/2Ā phase difference: just rotate the animation above by 90 degrees, or think about the formula: sinφ = cos(Ļ†āˆ’Ļ€/2). šŸ™‚

So A = A0Ā·cos(ωt + Īø) is the amplitude. It could be the voltage, or the current, or whatever realĀ variable.Ā The phase vectorĀ itself is represented by a complex number, i.e. a two-dimensional number, so to speak, which we can write as all of the following:

A = A0Ā·eiφ = A0Ā·cosφ + iĀ·A0Ā·sinφ = A0Ā·cos(ωt+Īø) + iĀ·A0Ā·sin(ωt+Īø)

=Ā A0Ā·ei(ωt+Īø)Ā = A0Ā·eiĪøĀ·eiωtĀ = A0Ā·eiωtĀ with A0Ā = A0Ā·eiĪø

That’s just Euler’s formula, and I am afraid I have to refer you to my page on theĀ essentialsĀ if you don’t get this. I know what you are thinking: why do we need the vector notation? Why can’t we just be happy with the A = A0Ā·cos(ωt+Īø) formula? The truthful answer is: it’s just to simplify calculations: it’s easier to work with exponentials than with cosines or sines. For example, writingĀ ei(ωt + Īø)Ā = eiĪøĀ·eiωtĀ is easier than writing cos(ωt + Īø) = … […] Well? […]Ā Hmm… šŸ™‚

See!Ā You’re stuck already. You’d have to use the cos(α+β) = cosα·cosĪ²Ā āˆ’ sinα·sinβ formula: you’d get the same results (just do it for the simple calculation of theĀ impedanceĀ below) but it takes a lot more time, and it’s easier to make mistake. Having said why complex number notation is great, I also need to warn you. There are a few things you have to watch out for. One of these things is notation. The other is the kind of mathematical operations we can do: it’s usually alright but we need to watch out with the i2Ā = –1 thing when multiplyingĀ complex numbers. However, I won’t talk about that here because it would only confuse you even more. šŸ™‚

Just for the notation, let me note that Feynman would write A0Ā as A0Ā with the little hatĀ orĀ caretĀ symbol (∧) on top of it, so as to indicate the complexĀ coefficient isĀ notĀ a variable. So he writes A0Ā asĀ Ć‚0Ā =Ā A0Ā·eiĪø.Ā However, I find that confusing and, hence, I prefer using bold-type for any complex number, variable or not. The disadvantage is that we need to remember that the coefficient in front of the exponential is not a variable: it’s a complex number alright, but not a variable. Indeed, do look at thatĀ A0Ā = A0Ā·eiĪøĀ equality carefully: A0Ā is a specificĀ complex number that captures theĀ initial phase Īø. So it’s not the magnitude of the phasor itself, i.e. |A| =Ā A0. In fact, magnitude, amplitude, phase… We’re using a lot confusing terminology here, and so that’s why you need to ‘get’ the math.

The impedance is not a variable either. It’s some constant. Having said that, this constant will depend on theĀ angular frequency ω. So… Well… Just think about this as you continue to read. šŸ™‚ So the impedance is someĀ number, just like resistance, but it’s a complexĀ number. We’llĀ denote it by ZĀ and, using Euler’s formula once again, we’ll write it as:

Z =Ā |Z|eiĪøĀ = V/I = |V|ei(ωt +Ā ĪøV)/|I|ei(ωt +Ā ĪøI)Ā = [|V|/|I|]Ā·ei(ĪøVĀ āˆ’Ā ĪøI)

So, as you can see, it is,Ā literally, some complexĀ ratio, just like R = V/I was some realĀ ratio: it is a complex ratio because itĀ has a magnitude and a direction, obviously. Also please do note that, as I mentioned already, the impedance is, in general, some function of the frequency ω, as evidenced by the ωt term in the exponential, but so we’re not looking at ω as a variable: V and I are variables and, as such, they depend on ω, but so you should look at ω as some parameter. I know I should, perhaps, notĀ be so explicit on what’s going on, but I want to make sure you understand.

So what’s going on? The illustration below (credit goes to Wikipedia, once again) explains. It’s a pretty generic view of a very simple AC circuit. So we don’t care what the impedance is: it might be an inductor or a capacitor, or a combination of both, but we don’t care: we just call it an impedance, or an impedorĀ if you want. šŸ™‚ The point is: if we apply an alternating current, then the current and the voltage will both go up and down, but the current signal will lag the voltage signal, and some phase factor Īø tells us by how much, so Īø will be the phase difference.

General_AC_circuit

Now, we’re dividing one complex number by another in that Z = V/I formula above, and dividing one complex number by another is not allĀ thatĀ straightforward, so let me re-write that formula for Z above as:

V = Iāˆ—ZĀ = Iāˆ—|Z|eiĪø

Now, while that V = Iāˆ—Z formulaĀ resembles the V = IĀ·R formula, you should note the bold-face type for V and I, and theĀ āˆ— symbol I am using here for multiplication. TheĀ bold-face for V and I implies they’re vectors, or complex numbers. As for theĀ āˆ— symbol, that’s to make it clear we’re not talking a vector cross product AƗB here, but a product of two complex numbers. [It’s obviously notĀ a vector dot product either, because a vector dot product yields a real number, not some other vector.]

Now we write V and IĀ as you’d expect us to write them:

  • VĀ =Ā |V|ei(ωt +Ā ĪøV) = V0Ā·ei(ωt +Ā ĪøV)
  • IĀ =Ā |I|ei(ωt +Ā ĪøI)Ā = I0Ā·ei(ωt +Ā ĪøI)

ĪøVĀ andĀ ĪøIĀ are, obviously, the so-called initialĀ phase of the voltage and the current respectively. These ‘initial’ phases are notĀ independent: we’re talking a phaseĀ differenceĀ really, between the voltage and the current signal, and it’s determined by the properties of the circuit. In fact, that’s the whole point here: theĀ impedanceĀ is a property of the circuit and determines how theĀ current signal varies as a function of the voltage signal. In fact, we’ll often choose the t = 0 point such that ĪøVĀ and so then we need to find ĪøI. […]Ā OK. Let’s get on with it. Writing out all of the factors in the V = Iāˆ—ZĀ = Iāˆ—|Z|eiĪøĀ equation yields:

VĀ =Ā |V|ei(ωt +Ā ĪøV)Ā =Ā Iāˆ—ZĀ = |I|ei(ωt +Ā ĪøI)āˆ—|Z|eiĪøĀ = |I||Z|ei(ωt +Ā ĪøIĀ +Ā Īø)Ā 

Now, this equation must hold for all values of t, so we can equate the magnitudes and phases and, hence, the following equalities must hold:

  1. |V| =Ā |I||Z| ⇔ |Z| =Ā |V|/|I|
  2. ωt + ĪøVĀ =  ωt + ĪøIĀ + θ ⇔ θ = ĪøVĀ āˆ’ ĪøI

Done!Ā 

Of course, you’ll complain once again about those complex numbers: voltage and current are something real, isn’t it? And so what isĀ really aboutĀ this complex numbers? Well… I can just say what I said already. You’re right. I’ve used the complex notation only to simplify the calculus, so it’s only theĀ real partĀ of those complex-valued functions that counts.

OK. We’re done with impedance. We can now discuss the impedors, including resistors (for which we won’t haveĀ such lag or phase difference, but the concept of impedance applies nevertheless).

Before I start, however, you should think about what I’ve done above: IĀ explainedĀ the concept of impedance, but I didn’t do much with it. The real-life problem will usually be that you get the voltage as a function of time, and then you’ll have to calculate the impedance of a circuit and, then, the current as a function of time. So I just showed the fundamental relations but, in real life, you won’t know what Īø andĀ ĪøIĀ could possibly be. Well… Let me correct that statement: we’ll give you formulas forĀ Īø as we discuss the various circuit elements and their impedance below, and so then you can use these formulas to calculateĀ ĪøI. šŸ™‚

Resistors

Let’s start with what seems to be the easiest thing: a resistor. A real resistor is actually not easy to understand, because it requires us to understand the properties ofĀ realĀ materials. Indeed, it may or may not surprise you, but the linear relation between the voltage and the current for realĀ materials is only approximate.Ā Also, the way resistors dissipateĀ energy is not easy to understand. Indeed, unlike inductors and capacitors, i.e. the other twoĀ passiveĀ components of an electrical circuit, a resistor does not storeĀ butĀ dissipatesĀ energy, as shown below.

Electric_load_animation_2

It’s a nice animation (credit for it has to go to Wikipedia once more), as it shows how energy is being used in an electric circuit. Note that the little moving plusesĀ are in line with the conventionĀ that a current is defined as the movement of positive charges, so we write I = dQ/dt instead ofĀ I =Ā āˆ’dQ/dt. That also explains the direction of the field line E, which has been added to show that the charges move with the field that is being generatedĀ by theĀ power source (which is not shown here). So, what we have here is that, on one side of the circuit, someĀ generator or voltage sourceĀ will create anĀ emfĀ pushing the charges,Ā and so the animation shows how someĀ load – i.e. the resistor in this case – willĀ consumeĀ their energy, so they lose their push (as shown by the change in color from yellow to black). SoĀ power, i.e.energy per unit time, is supplied, and is then consumed.

To increase the current in the circuit above, you need to increase the voltage, but increasing both amounts to increasing the powerĀ that’s being consumed in the circuit. Electric power is voltage times current, so P = VĀ·I (or vĀ·i, if I use the small letters that are used in the two animations below). Now, Ohm’s LawĀ (I = V/R)Ā says that, if we’d want to double the current, we’d need to double the voltage, and so we’re quadrupling the power then: P2Ā = V2Ā·I2Ā = (2Ā·V1)Ā·(2Ā·I1) = 4Ā·V1Ā·I1Ā = 22Ā·P1. So we have a square-cube law for the power, which we get by substituting V for RĀ·I or by substituting I for V/R, so we can write the power P as P = V2/R = I2Ā·R. This square-cube law says exactly the same: if you want to doubleĀ the voltageĀ orĀ the current, you’ll actually have to double both and, hence, you’ll quadruple the power.

But back to the impedance: Ohm’s Law is theĀ Z = V/I law for resistors, but we can simplify it because we know the voltage acrossĀ the resistorĀ and the current that’s going throughĀ areĀ in phase. Hence, ĪøVĀ andĀ ĪøIĀ are identical and, therefore, theĀ Īø = ĪøVĀ āˆ’ ĪøIĀ in Z =Ā |Z|eiĪøĀ is equal to zero and, hence, Z =Ā |Z|. Now,Ā |Z| =Ā |V|/|I| =Ā V0/I0. So the impedanceĀ ZĀ is just some real number R = V0/I0, which we can also write as:

R = V0/I0Ā = (V0Ā·ei(ωt + α))/(I0Ā·ei(ωt + α)) = V(t)/I(t), with α = ĪøVĀ = ĪøI

The equation above goes from R = V0/I0Ā to R = V(t)/I(t) = V/I. It’s note the same thing: the second equation says that,Ā at any point in time, the voltage and the current will be proportional to each other, with R or its reciprocal as the proportionality constant. In any case,Ā we have our formula for ZĀ here:

Z = R = V/I =Ā V0/I0

So that’s simple. Before we move to the next, let me note that the resistance of aĀ realĀ resistor may depend on itsĀ temperature, so in real-life applications one will want to keep its temperature as stable as possible. That’s why real-life resistors have power ratings and recommended operatingĀ temperatures. The image below illustrates how so-called heat-sink resistors can be mounted on a heat sink with a simple spring clip so as to ensureĀ the dissipated heat is transported away. These heat-sink resistors are rather small (10 by 15 mm only) but are rated for 35Ā watt – so that’s quite a lot for such small thing – ifĀ correctly mounted.

spring-clips-mounting-technigques

As mentioned, the linear relation between the voltage and the current is onlyĀ approximate, and the observed relation is also there only for frequencies that are not ‘too high’ because, if the frequency becomes very high, the free electrons will start radiating energy away, as they produce electromagnetic radiation. So one always needs to look at the tolerances of real-lifeĀ resistors, which may be ± 5%, ± 10%, or whatever.Ā In any case… On to the next.

Capacitors (condensers)

We talked at length about capacitors (aka condensers) in our post explaining capacitanceĀ or, the more widely used term, capacity: theĀ capacity of a capacitor is the observedĀ proportionality between (1) the voltage (V) across and (2) the charge (Q) on the capacitor, so we wrote it as:

C = Q/V

Now, it’s easy to confuse the C here with the C for coulomb, which I’ll also use in a moment, and so… Well… Just don’t! šŸ™‚ The meaning of the symbol is usually obvious from the context.

As for the explanation of this relation, it’s quite simple: a capacitor consists of two separateĀ conductors in space, with positive charge on one, and an equal and opposite (i.e. negative) charge on the other. Now, the logic of the superposition of fields implies that, if we double the charges, we will also double the fields, and so the work one needs to do to carry a unit charge from one conductor to the other is also doubled! So that’s why the potential difference between the conductors is proportional to the charge.

The C = Q/VĀ formula actually measures theĀ ability of the capacitor to store electric charge and, therefore, to store energy, so that’s why the term capacityĀ is really quite appropriate.Ā I’ll let youĀ googleĀ a few illustrations like the one below, that shows how a capacitor is actually being charged in a circuit. Usually, some resistance will be there in the circuit, so as to limit the current when it’s connected to the voltage source and, therefore, as you can see, the R times C factor (RĀ·C) determines how fast or how slow the capacitor charges and/or discharges. Also note that the current is equal to the time rate of change of the charge: I = dQ/dt.

images

In the above-mentioned post, we also give a few formulas for the capacity of specificĀ typesĀ of condensers. For example, for aĀ parallel-plate condenser, the formula was CĀ =  ε0A/d. We also mentioned its unit, which is isĀ coulomb/volt, obviously, but – in honor of Michael Faraday, who gave us Faraday’s Law, and many other interesting formulas – it’s referred to as theĀ farad: 1 F = 1 C/V. The C here isĀ coulomb, of course. Sorry we have to use C to denote two different things but, as I mentioned, the meaning of the symbol is usually clear from the context.

We also talked about how dielectrics actually work in that post, but we did notĀ talk about the impedance of a capacitor, so let’s do that now. The calculation is pretty straightforward. Its interpretation somewhat less so. But… Well… Let’s go for it.

It’s the current that’s charging the condenser (sorry I keep using both terms interchangeably), and we know that the current is the time rate of change of the charge (I = dQ/dt).Ā Now, you’ll remember that, in general, we’d write a phasor A as A = A0Ā·eiωtĀ with A0Ā = A0Ā·eiĪø, soĀ A0Ā is a complex coefficient incorporating the initial phase, which we wrote as ĪøVĀ andĀ ĪøIĀ for the voltage and for the current respectively. So we’ll represent the voltage and the current now using that notation, so we write: V = V0Ā·eiωtĀ and I = I0Ā·eiωt. So let’s now use that C = Q/V by re-writing it as Q = CĀ·V and, because C is some constant, we can write:

I = dQ/dt = d(CĀ·V)/dt = CĀ·dV/dt

Now, what’s dV/dt? Oh… You’ll say: V is the magnitude of V, so it’s equal toĀ |V| = |V0Ā·eiωt| = |V0|Ā·|eiωt| = |V0| = |V0Ā·eiĪø| =Ā |V0|Ā·|eiĪø| =Ā |V0| = V0. So… Well…Ā What?Ā V0Ā is some constant here! It’s theĀ maximumĀ amplitude of V, so… Well… It’s time derivative is zero: dV0/dt = 0.

Yes. Indeed. We did something very wrong here!Ā You really need to watch out with this complex-number notation, and you need to think about what you’re doing. V is not the magnitude of V but its (varying) amplitude. So it’s theĀ realĀ voltage V that varies with time: it’s equal to V0Ā·cos(ωt + ĪøV), which is the realĀ part of our phasorĀ V. Huh?Ā Yes.Ā Just hang in for a while. I know it’s difficult and, frankly, Feynman doesn’t help us very much here.Ā Let’s take one step back and so – you will see why I am doing this in a moment – let’s calculate the time derivative of our phasor V, instead of the time derivative of our realĀ voltageĀ V. So we calculate dV/dt, which is equal to:

dV/dtd(V0Ā·eiωt)/dt =Ā V0Ā·d(eiωt)/dt = V0Ā·(iω)Ā·eiωtĀ = iω·V0Ā·eiωtĀ = iω·V

Remarkable result, isn’t it? We take the time derivative of our phasor, and the result is the phasor itself multiplied with iω. Well… Yes. It’s a general property of exponentials, but still… Remarkable indeed! We’d get the same with I, but we don’t need that for the moment. What we doĀ need to do is go from ourĀ I =Ā CĀ·dV/dtĀ relation, which connects theĀ realĀ parts of I and V one to another, to theĀ I =Ā CĀ·dV/dtĀ relation, which relates theĀ (complex) phasors. So we write:

Ā I =Ā CĀ·dV/dt ⇔ I =Ā CĀ·dV/dt

Can we do that? Just like that? We just replace I and V by I and V? Yes, we can.Ā Why? Well… We know that I is the real part ofĀ I and so we can write I = Re(I)+ Im(I)Ā·i = I + Im(I)Ā·i, and then we can write the right-hand side of the equation as CĀ·dV/dt = Re(CĀ·dV/dt)+ Im(CĀ·dV/dt)Ā·i. Now, two complex numbers are equal if, and only if, their real and imaginary parts are the same, so… Well… Write it all out, if you want, using Euler’s formula, and you’ll see it all makes sense indeed.

So what do we get? TheĀ I =Ā CĀ·dV/dt gives us:

I =Ā CĀ·dV/dt = CĀ·(iω)Ā·V

That implies that I/V = CĀ·(iω) and, hence, we get – finally! – what we need to get:

Z = V/I = 1/(iωC)

This is a grand result and, while I am sorry I made you suffer for it, I think it did a good job here because, if you’d check Feynman on it, you’ll see he – or, more probably, his assistants, – just skate over this without bothering too much about mathematical rigor. OK.Ā All that’s left now is to interpret this ‘number’ Z = 1/(iωC). It is a purelyĀ imaginary number, and it’s a constant indeed, albeit a complex constant. ItĀ can be re-written as:

Z = 1/(iωC) = i-1/(ωC) = –i/(ωC) = (1/ωC)Ā·eāˆ’iĀ·Ļ€/2

[Sorry. I can’t be more explicit here. It’s just of the wonders of complex numbers: i-1 = –i. Just check one my posts on complex numbers for more detail.] Now, a –iĀ factor corresponds to a rotation ofĀ minusĀ 90 degrees, and so that gives you the true meaning of what’s usually said about a circuit with a capacitor:Ā the voltage across the capacitor willĀ lagĀ the current with a phase differenceĀ equal to π/2, as shown below. Of course, as it’s the voltage driving the current, we should say it’s the current that is lagging with a phase difference of 3Ļ€/2, rather than stating it the other way around! Indeed, i-1 = –i = –1Ā·i =Ā i2Ā·i = i3, so that amounts to three ‘turns’ of the phase in the counter-clockwise direction, which is the direction in which our ωt angle is ‘turning’.

800px-VI_phase

It is a remarkable result, though. The illustration above assumes the maximum amplitude of the voltage and the current are the same, soĀ |Z|Ā =Ā |V|/|I| = 1, but what if they are notĀ the same? What are the real bits then? I can hear you, indeed: “To hell with the bold-face letters: what’s V and I? What’s the realĀ thing?”

Well… V and I are the real bits ofĀ VĀ =Ā |V|ei(ωt+ĪøV) = V0Ā·ei(ωt+ĪøV)Ā and of IĀ =Ā |I|ei(ωt+ĪøI)Ā = I0Ā·ei(ωt+ĪøVāˆ’Īø)Ā =Ā I0Ā·ei(ωtāˆ’Īø)Ā = I0Ā·ei(ωt+Ļ€/2)Ā respectively so, assuming ĪøVĀ = 0 (as mentioned above, that’s just a matter of choosing a convenient t = 0 point), we get:

  • V = V0Ā·cos(ωt)
  • I = I0Ā·cos(ωt + Ļ€/2)

So the Ļ€/2 phase difference is there (you need to watch out with the signs, of course: Īø = āˆ’Ļ€/2, but so it’s the current that seems to leadĀ here)Ā but the V0/I0Ā ratio doesn’t have to be one, so the realĀ voltage and current could look like something below, where the maximumĀ amplitude of the current is only half of the maximumĀ amplitude of the voltage.

Capture

So let’s analyze this quickly: the V0/I0Ā ratio is equal to |Z| =Ā |V|/|I| = V0/I0Ā = 1/ωC = (1/ω)(1/C) (note that it’sĀ notĀ equal to V/I = V(t)/I(t), which is a ratio that doesn’t make sense because I(t) goes through zero as the current switches direction). So what? Well… It means the ratio is inversely proportional to both the frequency ω as well as the capacity C, as shown below. Think about this: if ω goes to zero, V0/I0Ā goes to āˆž, which means that, for a given voltage, the current must go to zero. That makes sense, because we’re talking DC current when ω → 0, and the capacitor charges itself and then that’s it: no more currents. Now, if C goes to zero, so we’re talking capacitors with hardly any capacity, we’ll also get tiny currents. Conversely, for large C, we’ll get huge currents, as the capacitor can take pretty much any charge you throw at it, so that makes for smallĀ V0/I0Ā ratios. The most interesting thing to consider is ω going to infinity, as the V0/I0Ā ratio is also quite small then. What happens? The capacitor doesn’t get the time to charge, and so it’s always in this state where it has large currents flowing in and out of it, as it can’t build the voltageĀ that would counter the electromotive force that’s being supplied by the voltage source.

graph 6OK. That’s it. Le’s discuss the last (passive) element.

Inductors

We’ve spoiled the party a bit with that illustration above, as it gives the phase difference for an inductor already:

Z = iωL = ωLĀ·eiĀ·Ļ€/2, with L the inductance of the coil

So, againĀ assuming thatĀ ĪøVĀ = 0, we can calculate I as:

IĀ =Ā |I|ei(ωt+ĪøI)Ā = I0Ā·ei(ωt+ĪøVāˆ’Īø)Ā =Ā I0Ā·ei(ωtāˆ’Īø)Ā = I0Ā·ei(ωtāˆ’Ļ€/2)Ā 

Of course, you’ll want to relate this, once again, to theĀ realĀ voltage and theĀ realĀ current, so let’s write the real parts of ourĀ phasors:

  • V = V0Ā·cos(ωt)
  • I = I0Ā·cos(ωt āˆ’ Ļ€/2)

Just to make sure you’re not falling asleep as you’re reading, I’ve made another graph of how things could look like. So now’s it’s the current signal that’sĀ lagging the voltage signalĀ with a phase differenceĀ equal toĀ Īø = Ļ€/2.

Capture

Also, to be fully complete, I should show you how the V0/I0Ā ratio now varies with L and ω. Indeed, here also we can write that |Z| =Ā |V|/|I| = V0/I0, but so here we find that V0/I0Ā =  ωL, so we have a simple linear proportionality here! For example, for a given voltage V0, we’ll have smallerĀ currents as ω increases, so that’s the opposite of what happens with our ideal capacitors. I’ll let you think about that… šŸ™‚

Capture

Now how do we get thatĀ Z = iωL formula? In my post on inductance, I explained what an inductor is: a coil of wire, basically. Its defining characteristic is thatĀ a changing current will cause a changingĀ magnetic field in it and, hence, some change in the flux of the magnetic field. Now, Faraday’s Law tells us that that will cause some circulation of the electric field in the coil, which amounts to an inducedĀ potential difference which is referred to as theĀ electromotive forceĀ (emf). Now, it turns out that the inducedĀ emfĀ is proportional to the change in current. So we’ve got another constant of proportionality here, so it’s like how we defined resistance, orĀ capacitance. So, in many ways, theĀ inductanceĀ is just another proportionality coefficient. If we denote it by L – the symbol is said to honor the Russian phyicistĀ Heinrich Lenz, whom you know from Lenz’ Law – then we define it as:

L = āˆ’Ę/(dI/dt)

The dI/dt factor is, obviously, the time rate of change of the current, and the negative sign indicates that the emfĀ opposesĀ the change in current, so it will tend to cause anĀ opposingĀ current. However, theĀ powerĀ of our voltage source will ensure the current does effectively change, so it will counter the ‘back emf’ that’s being generated by the inductor. To be precise, the voltage across the terminals of our inductor, which we denote by V, will be equal and opposite to ʐ, so we write:

V = āˆ’Ę = LĀ·(dI/dt)

Now, this very much resembles the I =Ā CĀ·dV/dt relation we had for capacitors, and it’s completely analogous indeed: we just need to switch the I and V, and C and L symbols. So we write:

Ā V = LĀ·dI/dt⇔ V = LĀ·dI/dt

Now, dI/dt is a similar time derivative as dV/dt. We calculate it as:

dI/dtd(I0Ā·eiωt)/dt =Ā I0Ā·d(eiωt)/dt = I0Ā·(iω)Ā·eiωtĀ = iω·I0Ā·eiωtĀ = iω·I

So we get what we want and have to get:

V = LĀ·dI/dt = iωLĀ·I

Now, Z = V/I, so Z =Ā iωL indeed!

Summary of conclusions

Let’s summarize what we found:

  1. For a resistor, we have Z(resistor) = ZRĀ = R = V/I =Ā V0/I0
  2. For an capacitor, we have Z(capacitor) = ZCĀ = 1/(iωC) = –i/(ωC)
  3. For an inductor, we haveĀ Z(inductance) = ZL= iωL

Note that the impedance of capacitors decreases as frequency increases, while for inductors, it’s the other way around. We explained that by making you think of the currents: for a given voltage, we’ll have large currents for high frequencies, and, hence, a smallĀ V0/I0Ā ratio. Can you think of what happens with an inductor? It’sĀ notĀ so easy, so I’ll refer you to the addendum below for some more explanation.

Let me also note that, as you can see, the impedance of (ideal) inductors and capacitors is a pure imaginary number, so that’s a complex number which has no real part. In engineering, the imaginary part of the impedance is referred to as theĀ reactance, so engineers will say that ideal capacitors and inductors have aĀ purely imaginary reactive impedance.Ā 

However, in real life, the impedance will usually have both a real as well as an imaginary part, so it will be some kind of mix, so to speak. The real part is referred to as the ‘resistance’ R, and the ‘imaginary’ part is referred to as the ‘reactance’ X. The formula for both is given below:

formula resistance and reactance

But here I have to end my post on circuit elements. It’s become quite long, so I’ll discuss Kirchoff’s rulesĀ in my next post.

Addendum: Why is V = āˆ’ ʐ?

Inductors are not easy to understand—intuitively, that is. That’s why I spent so much time writing on them in my other post on them, to which I should be referring you here. But let me recapitulate the key points. The key idea is that we’re pumping energy into an inductor when applying a current and, as you know, the time rate of change is power: P = dW/dt, so we’re talking power here too, which is voltageĀ timesĀ current: P = dW/dt = VĀ·I.Ā The illustration below shows what happens when anĀ alternating currentĀ is applied to the circuit with the inductor. So the assumption is that the current goes in one and then in the other direction, so I > 0, and then I < 0, etcetera. We’re also assuming some nice sinusoidal curve for the current here (i.e. the blue curve), and so we get what we get for U (i.e. the red curve), which is the energy that’s stored in the inductor really, as it tries to resist the changing current: the energy goes up and down between zero and some maximum amplitude that’s determined by the maximum current.

power 2

So, yes, building up current requires energy from some external source, which is used to overcome the ‘back emf’ in the inductor, and that energy is stored in the inductor itself. [If you still wonder why it’s stored in the inductor, think about the other question: where else would it be stored?]Ā HowĀ is stored? Look at the graph and think: it’s stored as kinetic energy of the charges, obviously. That explains why the energy is zero when the current is zero, and why the energy maxes out when the current maxes out. So, yes, it all makes sense! šŸ™‚

Let me give another example.Ā The graph below assumes the current builds up to some maximum. As it reaches its maximum, theĀ storedĀ energy will also max out. This example assumesĀ direct current, so it’s a DC circuit: the current builds up, but then stabilizes at some maximum that we can find by applying Ohm’s Law to the resistanceĀ of the circuit: I = V/R. Resistance? But we were talking an ideal inductor? We are. If there’s no other resistance in the circuit, we’ll have a short-circuit, so the assumption is that we doĀ have some resistance in the circuit and, therefore, we should also think of some energyĀ lossĀ to heat from the current in the resistance. If not, well… Your power source will obviously soon reach its limits. šŸ™‚

power

So what’s going on then?Ā We have someĀ changingĀ current in the coil but, obviously, some kind of inertia also: the coil itself opposes the change in current through the ‘back emf’. Now, it requires energy, or power, to overcome the inertia, so that’s the power that comes from our voltage source: it will offset the ‘back emf’, so we may effectively think of a little circuit with an inductorĀ and a voltage source, as shown below.

circuit with coil

But why do we write V = āˆ’Ā Ę? Our voltage source can have any voltage, can’t it? Yes. Sure. But so the coil will always provide anĀ emf that’s exactly theĀ oppositeĀ of this voltage. Think of it: we have someĀ voltage that’s being applied across the terminals of the inductor, and so we’ll have some current. A current that’s changing. And it’s that current will generate an emf that’s equal to Ɛ = –LĀ·(dI/dt). So don’t think of ʐ as some constant: it’s the self-inductance coefficient L that’s constant, but I (and, hence, dI/dt) and V are variable.

The point is: we cannot have any potential difference in a perfect conductor, which is what the terminals are: any potential difference, i.e. any electric field really, would cause huge currents. In other words, the voltage V and the emf Ɛ have to cancel each other out,Ā all of the time. If not, we’d have huge currents in the wires re-establishing the V = āˆ’Ę equality.

Let me use Feynman’s argument here. Perhaps that will work better. šŸ™‚ Our ideal inductor is shown below: it’s shielded by some metal box so as to ensure it does not interact with the rest of the circuit. So we have some current I, which we assume to be an AC current, and we know someĀ voltageĀ is needed toĀ causeĀ that current, so that’s the potential difference V between the terminals.

inductor

The total circulation of E – around the whole circuit – can be written as the sum of two parts:

Formula circulaton

Now, we know circulation of E can only be caused by someĀ changingĀ magnetic field, which is what’s going on in the inductor:

emf

So this change in the magnetic flux is what it causing the ‘back emf’, and so the integral on the left is, effectively, equal to ʐ, not minus Ɛ but +ʐ.Ā Now, the second integral is equal to V, because that’s the voltage V between the two terminals a and b. So the whole integral is equal toĀ 0 = ʐ +Ā V and, therefore, we have that:

VĀ = āˆ’Ā Ę = LĀ·dI/dt

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

The LiĆ©nard–Wiechert potentials and the solution for Maxwell’s equations

In my post on gauges and gauge transformations in electromagnetics, I mentioned the full and complete solution for Maxwell’s equations, using the electric and magnetic (vector) potential Φ and A. Feynman frames it nicely, so I should print it and put it on the kitchen door, so I can look at it everyday. šŸ™‚

frame

I should print the wave equation we derived in our previous post too. Hmm… Stupid question, perhaps, but why is there no wave equation above? I mean: in the previous post, we said the wave equation was the solution for Maxwell’s equation, didn’t we?Ā The answer is simple, of course: the wave equation is a solution for waves originating from some source and traveling through free space, so that’s a special case. Here we have everything. Those integrals ‘sweep’ all over space, and so that’sĀ realĀ space, which is full of moving charges and so there’s waves everywhere. So the solution above is far more general and captures it all: it’s the potential at every point in space, and at every point in time, taking into account whatever else is there, moving or not moving. In fact, it isĀ the general solutionĀ of Maxwell’s equations.

How do we find it? Well… I could copy Feynman’s 21stĀ LectureĀ but I won’t do that. The solution is based on the formula for Φ and A for a small blob of charge, and then the formulas above just integrate over all of space. That solution for a small blob of charge, i.e. a point charge really, was first deduced in 1898, by a French engineer: Alfred-Marie LiĆ©nard. However, his equations did not get much attention, apparently, because a German physicist, Emil Johann Wiechert, worked on the same thing and found the very same equations just two years later. That’s why they are referred to as theĀ LiĆ©nard-Wiechert potentials, so they both get credit for it, even if both of them worked it out independently. These are the equations:

electric potential

magnetic potential

Now, you may wonder why I am mentioning them, and you may also wonder how we get those integrals above, i.e. our general solution for Maxwell’s equations, from them. You can find the answer to your second question in Feynman’s 21st Lecture. šŸ™‚ As for the first question, I mention them because one can derive two other formulas for E and B from them. It’s the formulas that Feynman uses in his firstĀ Volume, when studying light:Ā E

B

Now you’ll probably wonder how we can get these twoĀ equations from theĀ LiĆ©nard-Wiechert potentials. They don’t look very similar, do they? No, they don’t. Frankly, I would like to give you the same answer as above, i.e. check it in Feynman’s 21st Lecture, but the truth is that the derivation is so long and tedious that even Feynman says one needs “a lot of paper and a lot of time” for that. So… Well… I’d suggest we just use all of those formulas and not worry too much about where they come from. If we can agree on that, we’re actually sort of finished with electromagnetism. All the chapters that follow Feynman’s 21stĀ LectureĀ are applicationsĀ indeed, so they do not add all that much to the coreĀ of the classicalĀ theory of electromagnetism.

So why did I write this post? Well… I am not sure. I guess I just wanted to sum things up for myself, so I can print it all out and put it on the kitchen door indeed. šŸ™‚ Oh, and now that I think of it, I should add one more formula, and that’s the formula for sphericalĀ waves (as opposed to theĀ planeĀ waves we discussed in my previous post). It’s a very simple formula, and entirely what you’d expect to see:

spherical wave

The S function is the source function, and you can see that the formula is a Coulomb-like potential, but with the retarded argument. You’ll wonder: what is ψ? Is it E or B or what? Well… You can just substitute: ψ can be anything. Indeed, Feynman gives a very general solution for any type ofĀ spherical wave here. šŸ™‚

So… That’s it, folks. That’s all there is to it. I hope you enjoyed it. šŸ™‚

Addendum: Feynman’s equation for electromagnetic radiation

I talked about Feynman’s formula for electromagnetic radiation before, but it’s probably good to quickly re-explain it here. Note that it talks about the electric field only, as the magnetic field is so tiny and, in any case, if we have E then we can find B. So the formula is:

E

The geometry of the situation is depicted below. We have some charge q that, we assume, is moving through space, and so it creates some field E at point P. TheĀ er‘Ā vector is the unit vector from P to Q, so it points at the charge. Well… It points to where the charge was at the time just a little while ago, i.e. at the timeĀ t – r‘/c. Why? Well… We don’t know where q is right now, because the field needs some time travel, we don’t know q right now, i.e. q at time t. It might be anywhere. Perhaps it followed some weird trajectory during the time r‘/c, like the trajectory below.

radiation formula

So our er‘Ā vector moves as the charge moves, and so it will also have velocity and, likely, some acceleration, but what we measure for its velocity and acceleration, i.e. the d(er‘)/dt and d2(er‘)/dt2Ā in that Feynman equation, is also theĀ retardedĀ velocity and theĀ retardedĀ acceleration. But look at the terms in the equation. The first two terms have a 1/r’2Ā in them, so these two effects diminish with the square of the distance. The first term is just Coulomb’s Law (note that the minus sign in front takes care of the fact that like chargesĀ repelĀ and so the E vector will point in the other way). Well… It is and it isn’t, because of the retarded time argument, of course. And so we have the second term, which sort of compensates for that. Indeed, the d(er‘)/dt is the time rate of change of er‘Ā and, hence, if r‘/c = Ī”t, then (r‘/c)Ā·d(er‘)/dt is a first-order approximation of Ī”er‘.

As Feynman puts it: “The second term is as though nature were trying to allow for the fact that the Coulomb effect is retarded, if we might put it very crudely. It suggests that we should calculate the delayed Coulomb field but add a correction to it, which is its rate of change times the time delay that we use. Nature seems to be attempting to guess what the field at the present time is going to be, by taking the rate of change and multiplying by the time that is delayed.”Ā In short, the first two terms can be written as E = āˆ’(q/4πε0)/r‘2Ā·[er‘Ā +Ā Ī”er‘] and, hence, it’s a sort of modified Coulomb Law that sort of tries to guess what the electrostatic field at P should be based on (a) what it is right now, and (b) howĀ q’s direction and velocity, as measured now, would change it.

Now, the third term has a 1/c2Ā factor in front but, unlike the other two terms, this effect doesĀ notĀ fall off with distance. So the formula belowĀ fully describes electromagnetic radiation, indeed, because it’sĀ the only important term when we get ‘far enough away’, with ‘far enough’ meaning that the parts that go as the square of the distance have fallen off so much that they’re no longer significant.

radiation formula 2Of course, you’re smart, and so you’ll immediately note that, as r increases, that unit vector keeps wiggling but that effect will also diminish. You’re right. It does, but in a fairly complicated way.Ā The acceleration ofĀ er‘Ā has two components indeed. One is the transverse or tangential piece, because the end of er‘Ā goes up and down, and the other is a radial piece because it stays on a sphere and so it changes direction. The radial piece is the smallest bit, and actually also varies as the inverse square ofĀ rĀ when rĀ is fairly large. The tangential piece, however, varies only inversely as the distance, so as 1/r. So, yes, the wigglings of er‘Ā look smaller and smaller, inversely as the distance, but the tangential piece is and remains significant, because it does not vary as 1/r2Ā but as 1/r only.Ā  That’s why you’ll usually see the law of radiation written in an even simpler way:

final law of radiation

This law reduces the whole effect to the component of the acceleration that is perpendicular to the line of sightĀ only. It assumes the distance is huge as compared to the distance over whichĀ the charge is moving and, therefore, that r‘ and r can be equated for all practical purposes. It also notes that the tangential piece is all that matters, and so it equatesĀ d2(er‘)/dt2Ā with ax/r. The whole thing is probably best illustrated as below: we have aĀ generatorĀ driving charges up and down in G – so it’s an antennaĀ really – and so we’ll measure a strong signal when putting the radiation detector D in position 1, but we’ll measure nothing in position 3. [The detector is, of course, another antenna, but with an amplifier for the signal.] But so here I am starting to talk about electromagnetic radiation once more, which wasĀ notĀ what I wanted to do here, if only because Feynman does a much better job at that than I could ever do. šŸ™‚radiator

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Traveling fields: the wave equation and its solutions

Pre-script (dated 26 June 2020): Our ideas have evolved into a full-blown realistic (or classical) interpretation of all things quantum-mechanical. In addition, I note the dark force has amused himself by removing some material. So no use to read this. Read my recent papers instead. šŸ™‚

Original post:

We’ve climbed a big mountain over the past few weeks, post by post, šŸ™‚ slowly gaining height, and carefully checking out the various routes to the top. But we are there now: we finally fully understand how Maxwell’s equations actuallyĀ work. Let me jot them down once more:

Maxwell's equations

As for how real or unreal the E and B fields are, I gave you Feynman’s answer to it, so… Well… I can’t add to that. I should just note, or remind you, that we have a fully equivalent description of it all in terms of the electric and magnetic (vector) potential Φ and A, and so we can ask the same question about Φ and A. They explain realĀ stuff, so they’reĀ real in that sense. That’s what Feynman’s answer amounts to, and I am happy with it. šŸ™‚

What I want to do here is show how we can get from those equations to some kind of wave equation: an equation that describes how a field actuallyĀ travelsĀ through space. So… Well…Ā Let’s first look at that very particular wave function we used in the previous post to prove that electromagnetic waves propagate with speedĀ c, i.e. the speed of light. The fields were very simple: the electric field hadĀ a y-component only, and the magnetic field a z-component only. Their magnitudes, i.e. their magnitude where the field had reached, as it fills the space traveling outwards,Ā were given in terms of J, i.e. the surface current density going in the positive y-direction, and the geometry of the situation is illustrated below.

equation

sheet of charge

The fields were, obviously, zero where the fields had not reached as they were traveling outwards. And, yes, I know that sounds stupid. But… Well… It’s just to make clear what we’re looking at here. šŸ™‚

We also showed how the wave would look like if we would turn off itsĀ First CauseĀ after some time T, so if the moving sheet of charge would no longer move after time T. We’d have the followingĀ pulse traveling through space, a rectangular shapeĀ really:

wavefrontWe can imagine more complicated shapes for the pulse, like the shape shown below. J goes from one unit to two units at time t =Ā t1Ā and then to zero at t =Ā t2. Now, the illustration on the right shows the electric field as a function of x at the time t shown by the arrow. We’ve seen this before when discussing waves: if the speed of travel of the wave is equal toĀ c, then x is equal to x = cĀ·t, and the pattern is as shown below indeed: it mirrors what happenedĀ at the source x/c secondsĀ ago. So we write:

equation 2

12

This idea of using theĀ retardedĀ time t’ = t āˆ’ x/c in the argument of a wave function f – or, what amounts to the same, using x āˆ’ c/t – is key to understanding wave functions. I’ve explained this in veryĀ simple language in a post for my kids and, if you don’t get this, I recommend you check it out. What we’re doing, basically, isĀ converting something expressed in time units intoĀ something expressed in distance units, or vice versa, using theĀ velocityĀ of the wave as the scale factor, so time and distance are bothĀ expressed in the same unit, which may be seconds, or meter.

To see how it works, suppose we addĀ some timeĀ Ī”t to the argument of our wave function f, so we’re looking at f[xāˆ’c(t+Ī”t)] now, instead of f(xāˆ’ct). Now, f[xāˆ’c(t+Ī”t)]Ā = f(xāˆ’ctāˆ’cĪ”t), so we’ll get a different valueĀ for our function—obviously! But it’s easy to see that we canĀ restore our wave function FĀ to its former value by alsoĀ adding some distanceĀ Ī”x =Ā cĪ”t to the argument. Indeed, if we do so, we get f[x+Ī”xāˆ’c(t+Ī”t)] = f(x+cĪ”t–ctāˆ’cĪ”t) = f(x–ct). You’ll say: t āˆ’ x/cĀ is not the same asĀ x–ct. It is and it isn’t: any function of x–ct is also a function of t āˆ’ x/c, because we can write:

capture

Here, I need to add something about the directionĀ of travel. The pulse above travel in the positive x-direction, so that’s why we haveĀ x minusĀ ct in the argument. For a wave traveling in the negative x-direction, we’ll have a wave function y = F(x+ct).Ā In any case, I can’t dwell on this, so let me move on.

Now, Maxwell’s equations in free or empty space, where are thereĀ no charges nor currentsĀ to interact with, reduce to:

Maxwell in free space

Now, how can we relate this set of complicated equations to a simple wave function? Let’s do the exercise for our simple EyĀ and BzĀ wave. Let’s start by writing out the first equation, i.e.Ā āˆ‡Ā·E = 0, so we get:

f1

Now, our wave does notĀ vary in the y and z direction, so none of the components, including EyĀ and EzĀ depend on y or z. It only varies in theĀ x-direction, soĀ āˆ‚Ey/āˆ‚y and āˆ‚Ez/āˆ‚z are zero. Note that the cross-derivatives āˆ‚Ey/āˆ‚z and āˆ‚Ez/āˆ‚y are also zero: we’re talking a plane wave here, the field varies only with x. However, because āˆ‡Ā·E = 0,Ā āˆ‚Ex/āˆ‚x must be zero and, hence, ExĀ must be zero.

Huh?Ā What?Ā How is that possible? You just said that our field doesĀ vary in the x-direction! And now you’re saying it doesn’t it? Read carefully. I know it’s complicated business, but it all makes sense. Look at the function: we’re talking Ey, notĀ Ex. EyĀ does vary as a function of x, but our field does not have an x-component, so ExĀ = 0. We have no cross-derivative āˆ‚Ey/āˆ‚x in the divergence of E (i.e. inĀ āˆ‡Ā·E = 0).

Huh?Ā What?Ā Let me put it differently.Ā E has three components: Ex,Ā EyĀ andĀ Ez, and we have three space coordinates: x, y and z, so we have nine cross-derivatives. What I am saying is that allĀ derivatives with respect to y and z are zero. That still leaves us with threeĀ derivatives:Ā āˆ‚Ex/āˆ‚x, āˆ‚Ey/āˆ‚x, andĀ āˆ‚Ey/āˆ‚x. So… Because all derivatives in respect to y and z are zero, and because of the āˆ‡Ā·E = 0 equation, we knowĀ thatĀ āˆ‚Ex/āˆ‚x must be zero.Ā So, to make a long story short, I did notĀ say anything aboutĀ āˆ‚Ey/āˆ‚x or āˆ‚Ez/āˆ‚x. These may still be whatever they want to be, and they may vary in more or in less complicated ways. I’ll give an example of that in a moment.

Having said that, I do agree that I was a bit quick in writing that, because āˆ‚Ex/āˆ‚x = 0, ExĀ must be zero too. Looking at the math only,Ā ExĀ is not necessarilyĀ zero: it might be some non-zero constant. So… Yes. That’s a mathematical possibility. The static field from some charged condenser plate would be an example of a constantĀ ExĀ field. However, the point is that we’re notĀ looking at such static fields here: we’re talking dynamicsĀ here, and we’re looking at a particular type of wave: we’re talking a so-called planeĀ wave. Now, the wave front of a plane wave is… Well… A plane. šŸ™‚ SoĀ ExĀ is zero indeed. It’s a general result for planeĀ waves: the electric field of a planeĀ wave will always be at right angles to the direction of propagation.

Hmm… I can feel your skepticism here. You’ll say I am arbitrarily restricting the field of analysis… Well… Yes. For the moment. It’s not a reasonableĀ restriction though. As I mentioned above, the field of a plane wave may still vary in both the y- and z-directions, as shown in the illustration below (for which the credit goes to Wikipedia), which visualizes the electric field of circularly polarized light. In any case, don’t worry too much about. Let’s get back to the analysis. Just note we’re talking plane waves here. We’ll talk about non-plane waves i.e.Ā incoherentĀ light waves later. šŸ™‚

circular polarization

So we have plane waves and, therefore, a so-called transverse E field which we can resolve in two components: EyĀ and Ez. However, we wanted to study a very simply EyĀ field only. Why? Remember the objective of this lesson: it’s just to show how we go from Maxwell’s equations to the wave function, and so let’s keep the analysis simple as we can for now: we can make it more general later.Ā In fact, ifĀ we do the analysis now for non-zero EyĀ and zero Ez, we can do a similar analysis forĀ non-zero EzĀ and zero Ey, and the general solution is going to be some superposition of two such fields, so we’ll have a non-zeroĀ EyĀ andĀ Ez. Capito? šŸ™‚ So let me write out Maxwell’s second equation, and use the results we got above, so I’llĀ incorporate the zero values for the derivatives with respect to y and z, and also the assumption that EzĀ is zero. So we get:

f3[By the way: note that, out of the nine derivatives, the curl involves only the (six) cross-derivatives. That’s linked to the neat separation between the curl and the divergence operator. Math is great! :-)]

Now, because of the flux rule (āˆ‡Ć—EĀ = ā€“āˆ‚B/āˆ‚t), we can (and should) equate the three components of āˆ‡Ć—E above with the three components of ā€“āˆ‚B/āˆ‚t, so we get:

f4

[In case you wonder what it is that I am trying to do, patience, please! We’ll get where we want to get. Just hang in there and read on.] Now, āˆ‚Bx/āˆ‚t = 0 and āˆ‚By/āˆ‚t = 0 do not necessarily imply that BxĀ andĀ ByĀ are zero: there might be some magnets and, hence, we may have some constant static field. However, that’s a matter of choosing a reference point or, more simply, assuming that empty space is effectively empty, and so we don’t have magnets lying around and so we assume that BxĀ andĀ ByĀ are effectively zero. [Again, we can always throw more stuff in when our analysis is finished, but let’s keep it simple and stupid right now, especially because the BxĀ = ByĀ = 0 is entirely in line with the ExĀ = EzĀ = 0 assumption.]

The equations above tell us what we know already: the E and B fields are at right angles to each other. However, note, once again, that this is a more general result for all planeĀ electromagneticĀ waves, so it’s not only that very special caterpillar or butterfly field that we’re looking at it. [If you didn’t read my previous post, you won’t get the pun, but don’t worry about it. You need to understand the equations, not the silly jokes.]

OK. We’re almost there. Now we need Maxwell’s last equation. When we write it out, we get the following monstrously lookingĀ set of equations:

f5

However, because of all of the equations involving zeroes above šŸ™‚ only āˆ‚Bz/āˆ‚x is notĀ equal to zero, so the whole set reduced to only simple equation only:

f6

Simplifying assumptions are great, aren’t they? šŸ™‚ Having said that, it’s easy to be confused. You should watch out for the denominators: a āˆ‚x and a āˆ‚t are two veryĀ different things. So we have two equations now involving first-orderĀ derivatives:

  1. āˆ‚Bz/āˆ‚t = āˆ’āˆ‚Ey/āˆ‚x
  2. āˆ’c2āˆ‚Bz/āˆ‚x = āˆ’āˆ‚Ey/āˆ‚t

So what? Patience,Ā please!Ā šŸ™‚ Let’s differentiate the first equation with respect to x and the second with respect to t. Why? Because… Well… You’ll see. Don’t complain. It’s simple. Just do it. We get:

  1. āˆ‚[āˆ‚Bz/āˆ‚t]/āˆ‚x = āˆ’āˆ‚2Ey/āˆ‚x2
  2. āˆ‚[āˆ’c2āˆ‚Bz/āˆ‚x]/āˆ‚t = āˆ’āˆ‚2Ey/āˆ‚x2

So we can equate the left-hand sides of our two equations now, and what we get is a differential equation of the second order that we’ve encountered already, when we were studying wave equations. In fact, itĀ isĀ the wave equation for one-dimensional waves:

f7In case you want to double-check, I did a few posts on this, but, if you don’t get this, well… I am sorry. You’ll need to do some homework. More in particular, you’ll need to do some homework on differential equations. The equation above is basically some constraintĀ on the functional form of Ey. More in general, if we see an equation like:

f8

then the function ψ(x, t) must be some function

solution

So any function ψ like that will work. You can check it out by doing the necessary derivatives and plug them into the wave equation. [In case you wonder how you should go about this, Feynman actually does it for you in his Lecture on this topic, so you may want to check it there.]

In fact, the functionsĀ f(x āˆ’ c/t) andĀ g(x + c/t) themselves will also work as possible solutions. So we can drop one or the other, which amounts to saying that our ‘shape’ has to travel in some direction, rather than in both at the same time.Ā šŸ™‚ Indeed, from all of my explanations above, you know whatĀ f(x āˆ’ c/t) represents: it’s a wave that travels in the positive x-direction. Now, it may be periodic, but it doesn’tĀ haveĀ to be periodic. TheĀ f(x āˆ’ c/t) function could representĀ any constant ‘shape’Ā that’s traveling in the positive x-direction at speed c. Likewise, theĀ g(x + c/t) function could representĀ any constant ‘shape’Ā that’s traveling in the negativeĀ x-direction at speed c. As for super-imposing both…

Well… I suggest you check that post I wrote for my son, Vincent. It’s on the math of waves, but it doesn’t have derivatives and/or differential equations. It just explains how superimposition and all that works. It’s not very abstract, as it revolves around a vibrating guitar string. So, if you have trouble with all of the above, you may want to read that first. šŸ™‚ The bottom line is that we can get anyĀ wavefunction we want by superimposing simple sinusoidals that are traveling in one or the other direction, and so that’s what’s the more general solution really says. Full stop. So that’s what’s we’re doing really: we add very simple waves to get very more complicated waveforms. šŸ™‚

Now, I could leave it at this, but then it’s veryĀ easy to just go one step further, and that is to assume that EzĀ and, therefore, ByĀ are not zero. It’s just a matter of super-imposing solutions. Let me just give you the general solution. Just look at it for a while. If you understood all that I’ve said above, 20 seconds or so should be sufficient to say: “Yes, that makes sense. That’s the solution in two dimensions.” At least, I hope so! šŸ™‚

General solution two dimensions

OK. I should really stop now. But… Well… Now that we’ve got a general solution for all plane waves, why not be even bolder and think about what we could possibly say aboutĀ three-dimensionalĀ waves? So then ExĀ and, therefore, BxĀ would not necessarily be zero either. After all, light can behave that way. In fact, light is likely to beĀ non-polarizedĀ and, hence, ExĀ and, therefore, BxĀ are most probably not equal toĀ zero!

Now, you may think the analysis is going to be terribly complicated. And you’re right. It would beĀ if we’d stick to our analysis in terms of x, y and z coordinates. However, it turns out that the analysis in terms of vector equations is actually quite straightforward. I’ll just copy the Master here, so you can see His Greatness. šŸ™‚

waves in three dimensions

But what solution does an equation like (20.27) have? We can appreciate it’s actually three equations, i.e. one for each component, and so… Well… Hmm… What can we say about that? I’ll quote the Master on this too:

“How shall we find the general wave solution? The answer is that all the solutions of the three-dimensional wave equation can be represented as a superposition of the one-dimensional solutions we have already found. We obtained the equation for waves which move in the x-direction by supposing that the field did not depend on yĀ andĀ z. Obviously, there are other solutions in which the fields do not depend on xĀ andĀ z, representing waves going in the y-direction. Then there are solutions which do not depend on xĀ andĀ y, representing waves travelling in the z-direction. Or in general, since we have written our equations in vector form, the three-dimensional wave equation can have solutions which are plane waves moving in any direction at all. Again, since the equations are linear, we may have simultaneously as many plane waves as we wish, travelling in as many different directions. Thus the most general solution of the three-dimensional wave equation is a superposition of all sorts of plane waves moving in all sorts of directions.”

It’s the same thing once more:Ā we add very simple waves to get very more complicated waveforms. šŸ™‚

You must have fallen asleep by now or, else, be watching something else. Feynman must have felt the same.Ā After explaining all of the nitty-gritty above, Feynman wakes up his students. He does so by appealing to their imagination:

“Try to imagine what the electric and magnetic fields look like at present in the space in this lecture room. First of all, there is a steady magnetic field; it comes from the currents in the interior of the earth—that is, the earth’s steady magnetic field. Then there are some irregular, nearly static electric fields produced perhaps by electric charges generated by friction as various people move about in their chairs and rub their coat sleeves against the chair arms. Then there are other magnetic fields produced by oscillating currents in the electrical wiring—fields which vary at a frequency of 6060Ā cycles per second, in synchronism with the generator at Boulder Dam. But more interesting are the electric and magnetic fields varying at much higher frequencies. For instance, as light travels from window to floor and wall to wall, there are little wiggles of the electric and magnetic fields moving along at 186,000Ā miles per second. Then there are also infrared waves travelling from the warm foreheads to the cold blackboard. And we have forgotten the ultraviolet light, the x-rays, and the radiowaves travelling through the room.

Flying across the room are electromagnetic waves which carry music of a jazz band. There are waves modulated by a series of impulses representing pictures of events going on in other parts of the world, or of imaginary aspirins dissolving in imaginary stomachs. To demonstrate the reality of these waves it is only necessary to turn on electronic equipment that converts these waves into pictures and sounds.

If we go into further detail to analyze even the smallest wiggles, there are tiny electromagnetic waves that have come into the room from enormous distances. There are now tiny oscillations of the electric field, whose crests are separated by a distance of one foot, that have come from millions of miles away, transmitted to the earth from the Mariner II space craft which has just passed Venus. Its signals carry summaries of information it has picked up about the planets (information obtained from electromagnetic waves that travelled from the planet to the space craft).

There are very tiny wiggles of the electric and magnetic fields that are waves which originated billions of light years away—from galaxies in the remotest corners of the universe. That this is true has been found by ā€œfilling the room with wiresā€ā€”by building antennas as large as this room. Such radiowaves have been detected from places in space beyond the range of the greatest optical telescopes. Even they, the optical telescopes, are simply gatherers of electromagnetic waves. What we call the stars are only inferences, inferences drawn from the only physical reality we have yet gotten from them—from a careful study of the unendingly complex undulations of the electric and magnetic fields reaching us on earth.

There is, of course, more: the fields produced by lightning miles away, the fields of the charged cosmic ray particles as they zip through the room, and more, and more. What a complicated thing is the electric field in the space around you! Yet it always satisfies the three-dimensional wave equation.”

So… Well… That’s it for today, folks. šŸ™‚ We have some more gymnastics to do, still… But we’re really there. Or here, I should say: on top of the peak. What a view we have here! Isn’t it beautiful? It took us quite some effort to get on top of this thing, and we’re still trying to catch our breath as we struggle with what we’ve learned so far, but it’s really worthwhile, isn’t it? šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

A post for Vincent: on the math of waves

Pre-scriptum (dated 26 June 2020): These posts on elementary math and physics for my kids (they are 21 and 23 now and no longer need such explanations) have not suffered much the attack by the dark force—which is good because I still like them. While my views on the true nature of light, matter and the force or forces that act on them have evolved significantly as part of my explorations of a more realist (classical) explanation of quantum mechanics, I think most (if not all) of the analysis in this post remains valid and fun to read. In fact, I find the simplest stuff is often the best. šŸ™‚

Original post:

I wrote this post to just briefly entertain myself and my teenage kids. To be precise, I am writing this for Vincent, as he started to study more math this year (eight hours a week!), and as he also thinks he might go forĀ engineering studies two years from now. So let’s see if he gets this and āˆ’ much more importantlyĀ āˆ’Ā if he likes the topic. If not… Well… Then he should get even better at golf than he already is, so he can make a living out of it. šŸ™‚

To be sure, nothing what I write below requires an understanding of stuff you haven’t seen yet, like integrals, or complex numbers. There’s no derivatives, exponentials or logarithms either: you just need to know what a sine or a cosine is, and then it’s just a bit of addition and multiplication. So it’s just… Well… Geometry and waves as I would teach it to an interested teenager. So let’s go for it.Ā And, yes,Ā I am talking to you now, Vincent!Ā šŸ™‚

The animation below shows a repeatingĀ pulse. It is a periodic function: a traveling wave. It obviously travels in the positive x-direction, i.e. from left to right as per our convention. As you can see, theĀ amplitudeĀ of our little wave varies as a function of time (t) and space (x), so it’s a function in two variables, like y = F(u, v). You know what that is, and you also know we’d refer to y as the dependent variable and to u and v as the independentĀ variables.

pulse

Now, because it’s a wave, and because it travels in the positive x-direction, the argument of the wave function FĀ will be xāˆ’ct, so we write:

y = F(xāˆ’ct)

Just to make sure: c isĀ the speed of travel of this particular wave, so don’t think it’s the speed of light. This wave can be any wave: a water wave, a sound wave,… Whatever. Our dependentĀ variableĀ y is the amplitude of our wave, so it’s the vertical displacementĀ āˆ’ up or down āˆ’ of whatever we’re looking at. As it’s a repeating pulse, y is zero most of the time, except when that pulse is pulsing. šŸ™‚

So what’s the wavelength of this thing?

[…] Come on, Vincent. Think! Don’t just look at this!Ā 

[…] I got it, daddy! It’s the distance between two peaks, or between the center of two successive pulses— obviously! šŸ™‚

[…]Ā Good! šŸ™‚ OK. That was easy enough.Ā Now look at the argument of this function once again:

F = F(xāˆ’ct)

We are not merely acknowledging here that F is some function of x and t,Ā i.e. some function varying in space and time. Of course, F is that too, so we can write:Ā y = F = F(x, t) = F(xāˆ’ct), but it’sĀ moreĀ than just some function: we’ve got a very special argument here,Ā xāˆ’ct, and so let’s start our little lesson by explaining it.

The xāˆ’ct argument is there because we’re talking waves, so that is something moving through space and time indeed. Now, what are we actuallyĀ doing when we write xāˆ’ct? Believe it or not, we’re basically converting something expressed in time units into something expressed in distance units. So we’re converting time into distance, so to speak. To see how this works, suppose we addĀ some timeĀ Ī”t to the argument of our function y = F, so we’re looking at F[xāˆ’c(t+Ī”t)] now, instead of F(xāˆ’ct). Now,Ā F[xāˆ’c(t+Ī”t)]Ā = F(xāˆ’ctāˆ’cĪ”t), so we’ll get a different valueĀ for our function—obviously! But it’s easy to see that we canĀ restore our wave function FĀ to its former value by alsoĀ adding some distanceĀ Ī”x =Ā cĪ”t to the argument. Indeed, if we do so, we get F[x+Ī”xāˆ’c(t+Ī”t)] = F(x+cĪ”t–ctāˆ’cĪ”t) = F(x–ct).Ā For example, if cĀ = 3 m/s, then 2 seconds of time correspond to (2 s)Ɨ(3 m/s) = 6 meters of distance.

The idea behind adding both some time Ī”tĀ as well as some distance Ī”x is that you’re traveling with the waveform itself, or with its phaseĀ as they say. So it’s like you’re riding on its crest or in its trough, or somewhere hanging on to it, so to speak. Hence, the speed of a wave is also referred to as itsĀ phase velocity, which we denote byĀ vpĀ =Ā c.Ā Now, let me make some remarks here.

First, there is theĀ directionĀ of travel. The pulses above travel in the positive x-direction, so that’s why we haveĀ x minusĀ ct in the argument. For a wave traveling in the negative x-direction, we’ll have a wave function y = F(x+ct). [And, yes, don’t be lazy, Vincent: please go through the Ī”x =Ā cĪ”t math once again to double-check that.]

The second thing you should note is that the speed of a regular periodic wave is equal to to the product of itsĀ wavelengthĀ and itsĀ frequency, so we write: vpĀ =Ā cĀ = λ·f, which we can also write as Ī» = c/f or f =Ā c/Ī». Now, you know we express the frequency in oscillations or cyclesĀ per second, i.e. in hertz: one hertzĀ is, quite simply, 1Ā sāˆ’1, so the unit of frequency is the reciprocal of the second. So the m/s and the Hz units in the fraction below give us a wavelengthĀ Ī» equal to Ī» =Ā (20 m/s)/(5/s) = 4 m. You’ll say that’s too simple but I just want to make sure you’ve got the basics right here.

Capture

The third thing is that, in physics, and in math, we’ll usually work with nice sinusoidal functions, i.e. sine or cosine functions. A sine and a cosine function are the same function but with aĀ phase differenceĀ of 90 degrees, so that’s Ļ€/2 radians.Ā That’s illustrated below: cosĪø = sin(Īø+Ļ€/2).

Circle_cos_sin

Now, when we converted time to distance by multiplying it with c, what we actually did was to ensure that the argument of our wavefunction F was expressed in one unitĀ only: the meter, so that’s theĀ distanceĀ unit in the international SI system of units. So that’s why we had to convert time to distance, so to speak.

The other option is to express all in seconds, so that’s in time units. So then we should measure distance in seconds, rather than meters, so to speak, and the corresponding argument is t–x/c, and our wave function would be written as y = G(t–x/c). Just go through the sameĀ Ī”x =Ā cĪ”t math once more: G[t+Ī”t–(x+Ī”x)/c] =Ā G(t+Ī”t–x/cāˆ’cĪ”t/c) =Ā G(t–x/c).

In short, we’re talking the same wave function here, soĀ F(xāˆ’ct) = G(tāˆ’x/c), but the argument of F is expressed in distance units, while the argument of G is expressed in time units. If you’d want to double-check what I am saying here, you can use the same 20 m/s wave example again: suppose the distance traveled is 100 m, so x = 100 m and x/cĀ = (100 m)/(20 m/s) = 5 seconds. It’s always important to check the units, and you can see they come out alright in both cases! šŸ™‚

Now, to go from F or G to our sine or cosine function, we need to do yet another conversion of units, as the argument of a sinusoidal function is some angleĀ Īø, not metersĀ orĀ seconds.Ā In physics, we refer toĀ Īø as theĀ phaseĀ of the wave function. So we need degrees or, more common now, radians, which I’ll explain in a moment.Ā Let me first jot it down:

y = sin(2Ļ€(x–ct)/Ī»)

So what are we doing here? What’s going on? Well… First, we divide x–ct by the wavelengthĀ Ī», so that’s the (x–ct)/Ī» in the argument of our sine function. So our ‘distance unit’ is no longer the meter but the wavelength of our wave, so we no longer measure inĀ meterĀ but in wavelengths. For example, if our argumentĀ x–ct was 20 m, and the wavelength of our wave is 4 m, we get (x–ct)/Ī» = 5 between the brackets. It’s just like comparing our length: ten years ago you were about half my size. Now you’re the same: one unit. šŸ™‚ When we’re saying that, we’re usingĀ myĀ length as the unit – and so that’s also yourĀ length unit now šŸ™‚Ā ā€“Ā rather than meters or centimeters.

Now I need to explain the 2Ļ€ factor, which is only slightly more difficult. Think about it: one wavelength corresponds to one full cycle, so that’s the full 360° of the circle below. In fact, we’ll express angles inĀ radians, and the two animations below illustrate what a radian really is: an angle of 1Ā rad defines an arc whose length, as measured on the circle, is equal to the radius of that circle. […] Oh! Please look at the animations as two separate things: they illustrate the same idea, but they’re notĀ synchronized, unfortunately! šŸ™‚
2pi-unrolledCircle_radians

So… I hope it all makes sense now: if we add one wavelength to the argument of our wave function, we should get the same value, and so it’s equivalent to adding 2Ļ€ to the argument of our sine function. Adding half a wavelength, or 35% of it, or a quarter, or twoĀ wavelengths, or e wavelengths, etcĀ is equivalent to adding π, orĀ 35%Ā·2Ļ€Ā ā‰ˆ 2.2, or 2Ļ€/4 = Ļ€/2, or 2Ā·2Ļ€ = 4Ļ€, or eĀ·2Ļ€, etc to it. So… Well… Think about it: to go from the argument of our wavefunction expressed as a number of wavelengthsĀ āˆ’ so that’s (x–ct)/Ī» – to the argument of our sine function, which is expressed in radians, we need to multiply by 2Ļ€.

[…] OK, Vincent. If it’s easier for you, you may want to think of the 1/Ī» and 2Ļ€ factors in the argument of theĀ sin(2Ļ€(x–ct)/Ī») function as scaling factors: you’d use a scaling factorĀ when you go from one measurement scale to another indeed. It’s like usingĀ vincentsĀ rather than meter. If oneĀ vincentĀ corresponds to 1.8 m, then we need to re-scale all lengths by dividingĀ them by 1.8 so as to express them inĀ vincents. Vincent ten year ago was 0.9 m, so that’s half a vincent: 0.9/1.8 = 0.5. šŸ™‚

[…] OK. […] Yes, you’re right: that’s rather stupid and makes nobody smile. Fine. You’re right: it’s time to move on to more complicated stuff. Now, read the following a couple of times. It’s my one and only message to you:

If there’s anything at all that you shouldĀ remember from all of the nonsense I am writing about in this physics blog, it’s thatĀ any periodic phenomenon, any motion really, can be analyzed by assuming that it is the sum of the motions of all the different modes of what we’re looking at, combined with appropriate amplitudes and phases.

It really is a most amazing thing—it’s something very deep and very beautiful connecting all of physics with math.

We often refer to these modes as harmonicsĀ and, in one of my posts on the topic, I explained how the wavelengths of the harmonics of a classical guitar string – it’s just an example – depended on the length of the string only. Indeed, if we denote the various harmonics by their harmonic number n = 1, 2, 3,… n,… and the length of the string by L, we have Ī»1Ā =Ā 2L = (1/1)Ā·2L, Ī»2Ā = L = (1/2)Ā·2L, Ī»3Ā =Ā (1/3)Ā·2L,… Ī»nĀ =Ā (1/n)Ā·2L. So they look like this:

620px-Harmonic_partials_on_strings

etcetera (1/8, 1/9,…,1/n,… 1/āˆž)

The diagram makes it look like it’s very obvious, but it’s an amazing fact: theĀ materialĀ of the string, or itsĀ tension, doesn’t matter. It’s just the length: simple geometry is all that matters! As I mentioned in my post on music and physics, this realization led to a somewhat misplaced fascination with harmonic ratios, which the Greeks thought could explain everything. For example, the Pythagorean model of the orbits of the planets would also refer to these harmonic ratios, and it took intellectual giants like Galileo and Copernicus to finally convince the PopeĀ that harmonic ratios are great, but that they cannot explainĀ everything. šŸ™‚ [Note:Ā When I say that theĀ materialĀ of the string, or itsĀ tension, doesn’t matter, I should correct myself: they do come into play whenĀ timeĀ becomes the variable. Also note that guitar strings are not the same length when strung on a guitar: the so-called bridge saddle is not in an exact right angle to the strings: this is a link to some close-up pictures of a bridge saddle on a guitar, just in case you don’t have a guitar at home to check.]

Now, I already explained the need to express the argument of a wave function in radians – because we’re talking periodicĀ functions and so we want toĀ use sinusoidals āˆ’ and how it’s just a matter of units really, and so how we can go from meter to wavelengths to radians. I also explained how we could do the same for seconds, i.e. for time. The key to convertingĀ distance units to time units, and vice versa, is the speed of the wave, or the phaseĀ velocity, which relates wavelength and frequency:Ā cĀ = λ·f. Now, as we have to express everything in radians anyway, we’ll usuallyĀ substitute the wavelength and frequency by theĀ wavenumberĀ and theĀ angular frequency so as to convert these quantities too to something expressed inĀ radians. Let me quickly explain how it works:

  1. The wavenumber k is equal to k = 2Ļ€/Ī», so it’s some number expressed inĀ radians per unit distance, i.e. radiansĀ per meter. In the example above, whereĀ Ī» was 4 m, we have k =Ā 2Ļ€/(4 m) = π/2 radiansĀ per meter. To put it differently, if our wave travels one meter, its phase Īø will change by π/2.
  2. Likewise, the angular frequency is ω = 2π·f = 2Ļ€/T. Using the same example once more, so assuming a frequency of 5 Hz, i.e. a periodĀ of one fifth of a second,Ā we have ω =Ā 2Ļ€/[(1/5)Ā·s] = 10Ļ€ per second. So the phase of our wave will change with 10 times π in one second. NowĀ thatĀ makes sense because, in one second, we have five cycles, and so that corresponds to 5 times 2Ļ€.

Note that our definition implies that Ī» = 2Ļ€/k, and that it’s also easy to figure out thatĀ our definition of ω, combined with the fĀ = c/λ relation, implies that ω = 2π·c/Ī» and, hence, that c = ω·λ/(2Ļ€) =Ā (ω·2Ļ€/k)/(2Ļ€) = ω/k.Ā OK. Let’s move on.

Using the definitions and explanations above, it’s now easy to see that we can re-write our y = sin(2Ļ€(x–ct)/Ī») as:

y = sin(2Ļ€(x–ct)/Ī») =Ā sin[2Ļ€(x–(ω/k)t)/(2Ļ€/k)] =Ā sin[(x–(ω/k)t)Ā·k)] =Ā sin(kx–ωt)

Remember, however, that we were talking some wave that was traveling in the positive x-direction. For theĀ negativeĀ x-direction, the equation becomes:

y = sin(2Ļ€(x+ct)/Ī») = sin(kx+ωt)

OK. That should be clear enough. Let’s go back to our guitar string. We can go from Ī» to k by noting that Ī» = 2L and, hence, we get the following for all of the various modes:

k = k1Ā = 2π·1/(2L) = Ļ€/L, k2Ā = 2π·2/(2L) = 2k, k3Ā =Ā 2π·3/(2L) = 3k,,… knĀ =Ā 2π·3/(2L) = nk,…

That gives us our grand result, and that’s that we can write some very complicated waveform ĪØ(x) as the sum of an infinite number of simple sinusoids, so we have:

ĪØ(x) =Ā a1sin(kx) + a2sin(2kx) + a3sin(3kx) + … + ansin(nkx) + … =Ā āˆ‘Ā ansin(nkx)

The equation above assumes we’re looking at the oscillation at some fixed point in time. If we’d be looking at the oscillation at some fixed point in space, we’d write:

Φ(t) = a1sin(ωt) + a2sin(2ωt) + a3sin(3ωt) + … + ansin(nωt) + … =Ā āˆ‘Ā ansin(nωt)

Of course, to represent some very complicated oscillation on our guitar string,Ā we can and should combine someĀ ĪØ(x) as well as some Φ(t) function, butĀ how do we do that,Ā exactly? Well… We’ll obviously need both theĀ sin(kx–ωt) as well as those sin(kx+ωt) functions, as I’ll explain in a moment. However, let me first make another small digression, so as to complete your knowledge of wave mechanics. šŸ™‚

We look at a wave as something that’s traveling through space and time at the same time. In that regard, I told you that the speedĀ of the wave is its so-calledĀ phase velocity, which we denoted as vpĀ = cĀ and which, as I explained above, is equal toĀ vpĀ =Ā cĀ = λ·fĀ = (2Ļ€/k)Ā·(ω/2Ļ€) = ω/k. The animation below (credit for it must go to Wikipedia—and sorry I forget to acknowledge the same source for the illustrations above) illustrates the principle: the speed of travel of the red dot is the phase velocity. But you can see that what’s going on here is somewhat more complicated: we have a series of wave packetsĀ traveling through space and time here, and so that’s where the concept of the so-calledĀ groupĀ velocity comes in: it’s the speed of travel of the green dot.

Wave_group

Now, look at the animation below. What’s going on here? The wave packet (or theĀ groupĀ or theĀ envelopeĀ of the wave—whatever you want to call it) moves to the right, but the phase goes to the left, as the peaks and troughs move leftward indeed. Huh?Ā How is that possible? And where is this wave going? Left or right? Can we still associate someĀ directionĀ with the wave here?Ā It looks like it’s traveling in both directions at the same time!

Wave_opposite-group-phase-velocity

The wave actually does travel in both directions at the same time. Well… Sort of. TheĀ point is actually quite subtle. When I started this post by writing that the pulses were ‘obviously’ traveling in the positive x-direction… Well… That’s actually notĀ so obvious. What is it that is traveling really? Think about an oscillating guitar string: nothing travels left or right really. Each point on the string just moves up and down. Likewise, if our repeated pulse is some water wave, then the water just stays where it is: it just moves up and down. Likewise, if we shake up some rope, the rope is not going anywhere: we just started some motionĀ that is traveling down the rope.Ā In other words, the phase velocity is just a mathematical concept. The peaks and troughs that seem to be traveling are just mathematical points that are ‘traveling’ left or right.

What about the group velocity? Is that a mathematical notion too? It is. The wave packet is often referred to as the envelopeĀ of the wave curves, for obviously reasons: they’re enveloped indeed. Well… Sort of. šŸ™‚ However, while both the phase and group velocity are velocities of mathematical constructs, it’s obvious that, if we’re looking at wave packets, the group velocity would be of more interest to us than the phase velocity. Think of those repeated pulses as real water waves, for example: while the water stays where it is (as mentioned, the water molecules just go up and down—more or less, at least), we’d surely be interested to know how fast these waves are ‘moving’, and that’s given by the groupĀ velocity, not the phase velocity. Still, having said that, the group velocity is as ‘unreal’ as the phase velocity: both are mathematical concepts. The only thing that’s ‘real’ is the up and down movement. Nothing travelsĀ in reality. Now, I shouldn’t digress too much here, but that’s why there’s no limit on the phase velocity: it can exceed the speed of light. In fact, in quantum mechanics, some real-life particle āˆ’ like an electron, for instance – will be represented by a complex-valuedĀ wave function, and there’s no reason to put some limit on the phase velocity. In contrast, theĀ groupĀ velocity will actually be the speed of the electron itself, andĀ that speed can, obviously, approach the speed of light – in particle accelerators, for example – but it can never exceed it. [If you’re smart, and you are, you’ll wonder: what about photons? Well…The classical and quantum-mechanical view of an electromagnetic wave are surelyĀ notĀ the same, but they do have a lot in common: both photons and electromagnetic radiation travel at the speedĀ c. Photons can do so because their rest mass is zero. But I can’t go into any more detail here, otherwise this thing will become way too long.]

OK. Let me get back to the issue at hand. So I’ll now revert to the simpler situation we’re looking at here, and so that’s theseĀ harmonicĀ waves, whose form is a simple sinusoidal indeed. The animation below (and, yes, it’s also from Wikipedia) is the one that’s relevant for this situation. You need to study it for a while to understand what’s going on. As you can see, the green wave travels to the right, the blue one travels to the left, and the red wave function is the sum of both.

Superpositionprinciple

Of course, after all that I wrote above, I should use quotation marks and write ‘travel’ instead of travel, so as to indicate there’s nothing traveling really, except for those mathematical points, but then no one does that, and so I won’t do it either. Just make sure you always think twice when reading stuff like this! Back to the lesson: what’s going on here?

As I explained, the argument of a wave traveling towards the negativeĀ x-direction will be x+ct. Conversely, the argument of a wave traveling in theĀ positiveĀ x-direction will be x–ct. Now, our guitar string is going nowhere, obviously: it’s like the red wave function above. It’s a so-called standing wave.Ā The red wave function has nodes, i.e. points where there is no motion—no displacement at all! Between the nodes, every point moves up and down sinusoidally, but the pattern of motion stays fixed in space.Ā So that’s the kind of wave function we want, and the animation shows us how we can get it.

Indeed, there’s a funnyĀ thing with fixed strings:Ā when a wave reaches the clamped end of a string, it will be reflected with a change in sign, as illustrated below: we’ve got that F(x+ct) wave coming in, and then it goes back indeed, but with the sign reversed.

Capture

The illustration above speaks for itself but, of course, once again I need to warn you about the use of sentences like ‘the wave reaches the end of the string’ and/or ‘the wave gets reflected back’. You know what it really means now: it’s some movementĀ that travels through space. […] In any case, let’s get back to the lesson once more:Ā how do we analyze that?

Easy: the red wave function is the sum of two waves: one traveling to the right, and one traveling to the left. We’ll call these componentĀ waves F and G respectively, so we have y = F(x, t) + G(x, t). Let’s go for it.

Let’s first assume the string isĀ notĀ held anywhere, so that we have an infinite string along which waves can travel in either direction. In fact, the most general functional form to capture the fact that a waveform can travel in any direction is to write the displacement y as the sum ofĀ twoĀ functions: one wave traveling one way (which we’ll denote by F, indeed), and the other wave (which, yes, we’ll denote by G) traveling the other way. From the illustration above, it’s obvious that the F wave is traveling towards the negativeĀ x-direction and, hence, its argument will be x+ct. Conversely, the G wave travels in theĀ positiveĀ x-direction, so its argument is x–ct.Ā So we write:

y = F(x, t) + G(x, t) = F(x+ct) + G(x–ct)

So… Well… We knowĀ that the string is actually not infinite, but that it’s fixed to two points. Hence, y is equal to zero there: y = 0. Now let’s choose the origin of our x-axis at the fixed end so as to simplify the analysis. Hence, where y is zero, x is also zero. Now, at x = 0, our general solution above for the infinite string becomes Ā y = F(ct) + G(āˆ’ct) = 0, for all values of t. Of course, that means G(āˆ’ct) must be equal to –F(ct). Now, that equality is there for all values of t. So it’s there for all values of ct and āˆ’ct. In short, that equality is valid for whatever value of the argument ofĀ G and –F. As Feynman puts it: ā€œGĀ of anything must be –FĀ of minus that same thing.ā€ Now, the ā€˜anything’ in G is its argument: x – ct, so ā€˜minus that same thing’ is –(x–ct) =Ā āˆ’x+ct. Therefore, our equation becomes:

y = F(x+ct) āˆ’Ā F(āˆ’x+ct)

So that’s what’s depicted in the diagram above: the F(x+ct) wave ā€˜vanishes’ behind the wall as the āˆ’Ā F(āˆ’x+ct) wave comes out of it.Ā Now, of course, so as to make sure our guitar string doesn’t stop its vibration after being plucked, we need to ensure F is a periodic function, like aĀ sin(kx+ωt) function. šŸ™‚ Why? Well… If this F and G function would simply disappear and ‘serve’ only once, so to speak, then we only have one oscillation and that’s it! So the waves need to continue and so that’s why it needs to be periodic.

OK. Can we just takeĀ sin(kx+ωt) and āˆ’sin(āˆ’kx+ωt) and add both? It makes sense, doesn’t it? Indeed, āˆ’sinα = sin(āˆ’Ī±) and, therefore, āˆ’sin(āˆ’kx+ωt) = sin(kxāˆ’Ļ‰t). Hence,Ā y = F(x+ct) āˆ’Ā F(āˆ’x+ct) would be equal to:

y =Ā sin(kx+ωt) + sin(kx–ωt) = sin(2Ļ€(x+ct)/Ī») + sin(2Ļ€(xāˆ’ct)/Ī»)

Done! Let’s use specific values for k and ω now. For the first harmonic, we know that k =Ā 2Ļ€/2L = Ļ€/L. What about ω? Hmm… That depends on the wave velocity and, therefore, that actually doesĀ dependĀ on the material and/or the tension of the string! The only thing we can say is that ω = cĀ·k, so ω =Ā cĀ·2Ļ€/Ī» = cĀ·Ļ€/L. So we get:

sin(kx+ωt) = sin(π·x/L + π·cĀ·t/L) =Ā sin[(Ļ€/L)Ā·(x+ct)]

But this is our F function only. The whole oscillation isĀ y = F(x+ct) āˆ’Ā F(āˆ’x+ct), and āˆ’Ā F(āˆ’x+ct) is equal to:

 –sin[(Ļ€/L)Ā·(āˆ’x+ct)] = –sin(āˆ’Ļ€Ā·x/L+π·cĀ·t/L) =Ā āˆ’sin(āˆ’kx+ωt) = sin(kx–ωt) =Ā sin[(Ļ€/L)Ā·(x–ct)]

So, yes, we should add both functions to get:

y = sin[Ļ€(x+ct)/L] + sin[Ļ€(xāˆ’ct)/L]

Now, we can, of course, apply our trigonometric formulas for the addition of angles, which say that sin(α+β) =Ā sinαcosβ + sinβcosα and sin(α–β) =Ā sinαcosβ – sinβcosα. Hence, y =Ā sin(kx+ωt) +Ā sin(kx–ωt) is equal toĀ sin(kx)cos(ωt) + sin(ωt)cos(kx) + sin(kx)cos(ωt) – sin(ωt)cos(kx) = 2sin(kx)cos(ωt). Now, that’s a very interesting result, so let’s give it some more prominence by writing it in boldface:

y =Ā sin(kx+ωt) +Ā sin(kx–ωt) =Ā 2sin(kx)cos(ωt) =Ā 2sin(π·x/L)cos(π·cĀ·t/L)

TheĀ sin(π·x/L) factor gives us the nodes in space. Indeed,Ā sin(π·x/L) = 0 ifĀ x is equal to 0 or L (values of x outside of the [0, L] interval are obviously notĀ relevant here). Now, the other factorĀ cos(π·cĀ·t/L) can be re-written cos(2π·cĀ·t/Ī») = cos(2π·fĀ·t) = cos(2π·t/T), with T the periodĀ T = 1/fĀ = Ī»/c, so the amplitude reaches a maximum (+1 orĀ āˆ’1 or, including the factor 2, +2 or āˆ’2) if 2π·t/T is equal to a multiple of Ļ€, so that’s ifĀ t = nĀ·T/2 with n = 0, 1, 2, etc. In our example above, for f = 5 Hz, that means the amplitude reaches a maximum (+2 or āˆ’2) every tenthĀ of a second.

The analysis for the other modes is as easy, and I’ll leave it you, Vincent,Ā as an exercise, to work it all out and send me the y = 2Ā·sin[something]Ā·cos[something else] formula (with the ‘something’ and ‘something else’ writtenĀ in terms of L and c, of course) for the higher harmonics.Ā šŸ™‚

[…] You’ll say: what’s the point, daddy? Well… Look at that animation again: isn’t it great we can analyze any standing wave, or any harmonic indeed, as the sum ofĀ twoĀ component waves with the same wavelength and frequency but ‘traveling’ in opposite directions?Ā 

Superpositionprinciple

Yes, Vincent. I can hear you sigh: “Daddy, I really do notĀ see why I should be interested in this.”

Well… Your call… What can I say? Maybe one day you will. In fact, if you’re going to go for engineering studies, you’ll have to. šŸ™‚

To conclude this post, I’ll insert one more illustration. Now that you know whatĀ modesĀ are, you can start thinking about those more complicatedĀ ĪØ and Φ functions. The illustration below shows how the first and second mode of our guitar string combine to give us some composite wave traveling up and down the very same string.

composite wave

Think about it. We haveĀ oneĀ physical phenomenon here: at every point in time, the string is somewhere, butĀ where exactly, depends on the mathematical shape of its components. If this doesn’t illustrate the beauty of Nature, the fact that, behind every simple physicalĀ phenomenon āˆ’ most of which are some sort of oscillation indeed āˆ’ we have some marvelous mathematicalĀ structure, then… Well… Then I don’t know how to explain why IĀ am absolutely fascinated by this stuff.

Addendum 1: On actual waves

My examples of waves above were all examples of so-called transverseĀ waves, i.e. oscillations at a right angle to the direction of the wave. The other type of wave is longitudinal. I mentioned sound waves above, but they are essentiallyĀ longitudinal. So thereĀ  the displacement of the medium is in the same direction of the wave, as illustrated below.Onde_compression_impulsion_1d_30_petit

Real-life waves, like water waves, may be neither of the two. The illustration below shows how water molecules actually move as a wave passes. They move in little circles, with a systemic phase shift from circle to circle.

Water waves

Why is this so? I’ll let Feynman answer, as he also provided the illustration above:

“Although the water at a given place is alternately trough or hill, it cannot simply be moving up and down, by the conservation of water. That is, if it goes down, where is the water going to go? The water is essentially incompressible. The speed of compression of waves—that is, sound in the water—is much, much higher, and we are not considering that now. Since water is incompressible on this scale, as a hill comes down the water must move away from the region. What actually happens is that particles of water near the surface move approximately in circles. When smooth swells are coming, a person floating in a tire can look at a nearby object and see it going in a circle. So it is a mixture of longitudinal and transverse, to add to the confusion. At greater depths in the water the motions are smaller circles until, reasonably far down, there is nothing left of the motion.”

So… There you go… šŸ™‚

Addendum 2: On non-periodic waves, i.e. pulses

A waveform isĀ notĀ necessarily periodic. The pulse we looked at could, perhaps,Ā not repeat itself. It is notĀ possible, then, to describe its wavelength. However, it’s still a wave and, hence, its functional form would still be some y = F(xāˆ’ct) or y = F(x+ct) form, depending on its direction of travel.

The example below also comes out of Feynman’s Lectures: electromagnetic radiation is caused by someĀ acceleratingĀ electric charge – an electron, usually, because its mass is small and, hence, it’s much easier to move than a proton šŸ™‚ – and then the electric field travels out in space.Ā So the two diagrams below show (i) the acceleration (a) as a function of time (t) and (ii) the electric field strength (E) as a function of the distance (r). [To be fully precise, I should add he ignores the 1/r variation, but that’s a fine point which doesn’t matter much here.]

EM 1EM 2 Ā Ā Ā 

He basically uses this illustration to explain why we can use a y =Ā G(t–x/c) functional form to describe a wave. The point is: he actually talks about oneĀ pulse only here. So theĀ F(x±ct) or G(t±x/c) or sin(kx±ωt) form hasĀ nothingĀ to do with whether or not we’re looking at a periodic or non-periodic waveform. The gist of the matter is that we’ve got something movingĀ through space, and it doesn’t matter whether it’s periodic or not: theĀ periodicity or non-periodicity,Ā of a wave has nothing to do with the x±ct, t±x/cĀ or kx±ωt shape of the argument of our wave function. The functional form of our argument is just the result of what I said about traveling along with our wave.

So what is it about periodicity then? Well… If periodicity kicks it, you’ll talk sinusoidal functions, and so the circle will be needed once more. šŸ™‚Ā Ā Ā 

Now, I mentioned we cannotĀ associate any particular wavelength with such non-periodic wave. Having said that, it’s still possible to analyze this pulseĀ as a sum ofĀ sinusoids through a mathematical procedure which is referred to as theĀ Fourier transform. If you’re going for engineer, you’ll need to learn how to master this technique. As for now, however, you can just have a look at the Wikipedia article on it. šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

The field from a grid

Pre-script (dated 26 June 2020): This post got mutilated by the removal of some material by the dark force. You should be able to follow the main story-line, however. If anything, the lack of illustrations might actually help you to think things through for yourself.

Original post:

As part of his presentation of indirect methods for finding the field, Feynman presents an interesting argument on the electrostatic field of a grid. It’s just another indirect method to arrive at meaningful conclusions on how a field is supposed to look like, but it’s quite remarkable, and that’s why I am expanding it here. Feynman’s presentation isĀ extremelyĀ succint indeed and, hence, I hope the elaboration below will helpĀ youĀ to understand it somewhat quicker than I did. šŸ™‚

The grid is shown below: it’s just a uniformly spaced array of parallel wires in a plane. We are looking at the field above the plane of wires here, and the dotted lines represent equipotentialĀ surfacesĀ above the grid.

grid

As you can see, for larger distances above the plane, we see a constant electric field, just as though the charge were uniformly spread over a sheet of charge, rather than over a grid. However, as we approach the grid, the field begins to deviate from the uniform field.

Let’s analyze it by assuming the wires lie in the xy-plane, running parallel to the y-axis. The distance between the wires is measured along the x-axis, and the distance to the grid is measured along the z-axis, as shown in the illustration above. We assume the wires are infinitely long and, hence, the electric field doesĀ notĀ depend on y. So the component of E in the y-direction is 0, so EyĀ = ā€“āˆ‚Ī¦/āˆ‚y = 0. Therefore,Ā āˆ‚2Φ/āˆ‚y2Ā = 0 and our Poisson equation above the wiresĀ (where there are no charges)Ā is reduced toĀ āˆ‚2Φ/āˆ‚x2Ā +Ā āˆ‚2Φ/āˆ‚z2Ā =0. What’s next?

Let’s look at the field of twoĀ positive wires first. The plot below comes from the Wolfram Demonstrations Project. I recommend you click the link and play with it: you can vary the charges and the distance, and the tool will redraw the equipotentials and the field lines accordingly. It will give you a better feel for the (a)symmetries involved. The equipotential lines are the gray contours: they are cross-sections of equipotential surfaces. The red curves are the field lines, which are always orthogonal to the equipotentials.

WolframThe point at the center is really interesting: the straight horizontal and vertical red lines through it are limits really. Feynman’s illustration below shows the point represents an unstableĀ equilibrium: the hollow tube prevents the charge from going sideways. So if it wouldn’t be there, the charge would go sideways, of course! So it’s some kind ofĀ saddleĀ point. Onward!hollow tube

Look at the illustration below and try to imagine how the field looks like by thinking about the value of the potential as you move along one of the two blue lines below: the potential goes down as we move to the right, reaches a minimum in the middle, and then goes up again. Also think about the difference between the lighter and darker blue line: going along the light-blue line, we start at a lowerĀ potential, and its minimum will also be lowerĀ than that of the dark-blue line.

lines

So you can start drawing curves. However, I have to warn you: the graphs areĀ notĀ so simple. Look at the detail below. The potential along the blue line goes slightly up before it decreases, so the graph of the potential may resemble the green curve on the right of the image. I did an actualĀ calculation here. šŸ™‚Ā If there are only two charges, the formula for the potential is quite simple: Φ = (1/4πε0)Ā·(q1/r1) +Ā (1/4πε0)Ā·(q2/r2). Briefly forgetting about the (1/4πε0) and equating q1Ā andĀ q2Ā to +1, we get Φ = 1/r1Ā + 1/r2Ā = (r1Ā + r2)/r1r2.Ā Ā That looks like an easy function, and it is. You should think of it as the equivalent of theĀ 1/r formula, but written as 1/r = r/r2, and with a factor 2 in front because we have two charges. šŸ™‚

However, we need to express it as a function of x, keeping z (i.e. the ‘vertical’ coordinate) constant. That’s what I did to get the graphs below. It’s easy to see that 1/r1Ā = (x2Ā +Ā z2)āˆ’1/2, while 1/r2Ā = [(aāˆ’x)2Ā + z2]āˆ’1/2. Assuming a = 2 and z = 0.8, the contribution from the first charge is given by the blue curve, the contribution of the second charge is represented by the red curve, and the green curve adds both and, hence, represents theĀ potentialĀ generated by both charges, i.e. q1Ā at x = 0 and q2Ā at x = a. OK… Onward!

Ā lines 3graph 2

The point to note is that we have anĀ extremely simple situation here – two charges only, or two wires, I should say – but a potential function that is surely notĀ some simple sinusoidal function. To drive the point home, IĀ plotted a few more curves below, keeping a at a = 2, but equating z with 0.4, 0.7 and 1.7 respectively. The z = 1.7 curve shows that, at larger distances, the potential actually increases slightly as we move from left to right along the z = 1.7 line. Note the remarkable symmetry of the curves and the equipotential lines: there should be some obvious mathematical explanation for that but, unfortunately, not obvious enough for me to find it, so please let me know if you see it! šŸ™‚

graph 3

OK. Let’s get back to our grid. For your convenience, I copied it once more below.

grid

Feynman’s approach to calculating the variations is quite original. He also duly notes that the potential function is surely notĀ some simple sinusoidal function. However, he also notes that, when everything is said and done, it is some periodic quantity, in one way or another, and, therefore, we should be able to do a Fourier analysisĀ andĀ express it as a sum of sinusoidal waves. To be precise, we should be able to write Φ(x, z) as a sum ofĀ harmonics.

[…] I know. […] Now you say:Ā Oh sh**! And you’ll just turn off. That’s OK, but why don’t you give it a try? I promise to be lengthy. šŸ™‚

Before we get too much into the weeds, let’s briefly recall how it works for our classical guitar string. That post explained how the wavelengths of the harmonics of a string depended on its length. If we denote the various harmonics by their harmonic number n = 1, 2, 3 etcetera, and the length of the string by L, we have Ī»1Ā =Ā 2L = (1/1)Ā·2L, Ī»2Ā = L = (1/2)Ā·2L, Ī»3Ā =Ā (1/3)Ā·2L,… Ī»nĀ =Ā (1/n)Ā·2L. In short, the harmonics – i.e. the componentsĀ of our waveform – look like this:

620px-Harmonic_partials_on_strings

etcetera (1/8, 1/9,…,1/n,… 1/āˆž)

Beautiful, isn’t it? As I explained in that post, it’s so beautiful it triggered a misplaced fascination with harmonic ratios. It was misplaced because the Pythagorean theory was a bit too simple to be true. However, their intuition was right, and they set the stage for guys like Copernicus, Fourier and Feynman, so that was good! šŸ™‚

Now, as you know, we’ll usually substitute wavelength and frequency by wavenumberĀ andĀ angular frequency so as to convert all to something expressed inĀ radians, which we can then use as the argument in the sine and/or cosine component waves. [Yes, the Pythagoreans once again! :-)] The wavenumber k is equal to k = 2Ļ€/Ī», and the angular frequency is ω = 2π·f = 2Ļ€/T (in case you doubt, you can quickly check that the speed of a wave cĀ is equal to the product of the wavelength and its frequency by substituting: cĀ = λ·fĀ = (2Ļ€/k)Ā·(ω/2Ļ€) = ω/k, which gives you the phaseĀ velocity vp= c). To make a long story short, we wrote k = k1Ā = 2π·1/(2L), k2Ā = 2π·2/(2L) = 2k, k3Ā =Ā 2π·3/(2L) = 3k,,… knĀ =Ā 2π·3/(2L) = nk,… to arrive at the grand result, and that’s our wave F(x) expressed as the sum of an infinite number of simple sinusoids:Ā 

F(x) =Ā a1cos(kx) + a2cos(2kx) + a3cos(3kx) + … + ancos(nkx) + … =Ā āˆ‘Ā ancos(nkx)

That’s easy enough. The problem is to find those amplitudes a1, a2, a3,… of course, but the great French mathematician who gave us the Fourier series also gave us the formulas for that, so we should be fine! Can we use them here? Should we use them here? Let’s see…

The aĀ in the analysis, i.e. the spacing of the wires, is the physical quantity that corresponds to the length of our guitar string in our musical sound problem. In fact, aĀ corresponds to 2L, because guitar strings are fixed at two ends and, hence, the two ends have to be nodes and, therefore, the wavelength of our first harmonic is twice the length of the string. Huh? Well… Something like that.Ā As you can see from the illustration of the grid, a, in contrast to L, does correspond toĀ oneĀ full wavelength of our periodic function. SoĀ we write:

Φ(x) = āˆ‘ ancos(nĀ·kĀ·x) =Ā āˆ‘ ancos(2π·nĀ·x/a) (n = 1, 2, 3,…)

Now, that’s the formula for Φ(x) assuming we’re fixingĀ z, so it’s Φ(x) at some fixed distance from the grid. Let’s think about those amplitudes anĀ now.Ā They should not depend on x, because the harmonics themselves (i.e. the cos(2π·nĀ·x/a) components) are all that varies with x. So they have be some function of n and – most importantly – some function of z also. So we denote them by Fn(z) and re-write the equation above as:

 Φ(x, z) = āˆ‘Ā Fn(z)Ā·cos(2π·nĀ·x/a)Ā (n = 1, 2, 3,…)

Now, the rest of Feynman’s analysis speaks for itself, so I’ll just shamelessly copy it:

Feynman

What did he find here? What is he saying, really? šŸ™‚ First note that the derivation above has been done for one term in the Fourier sum only, so we’re talking a specific harmonicĀ nĀ here.Ā ThatĀ harmonicĀ nĀ is a function of z which – let me remind you – is the distance from the grid. To be precise, the function is Fn(z) = Aneāˆ’z/z0. [In case you wonder how Feynman goes from equation (7.43) to (7.44), he’s just solving a second-order linear differential equation here. :-)]

Now, you’ve seen the graph of that function a zillion times before: it starts atĀ AnĀ for z = 0 and goes to zero as z goes to infinity, as shown below. šŸ™‚

graph 4

Now, that’s the case for allĀ Fn(z) coefficients of course. As Feynman writes:

“We have found that if there is a Fourier component of the field of harmonicĀ n, that component will decrease exponentially with a characteristic distance z0Ā = a/2Ļ€n. For the first harmonic (n=1), the amplitude falls by the factorĀ eāˆ’2π (i.e. a large decrease) each time we increaseĀ zĀ by one grid spacing a. The other harmonics fall off even more rapidly as we move away from the grid. We see that if we are only a few times the distanceĀ aĀ away from the grid, the field is very nearly uniform, i.e., the oscillating terms are small.Ā There would, of course, always remain the ā€œzero harmonicā€ field, i.e. Φ0Ā = āˆ’E0Ā·z, to give the uniform field at largeĀ z.Ā Of course, for the complete solution, the sum needs to be made, and the coefficients AnĀ would need to be adjusted so that the total sum, when differentiated, gives an electric field that would fit the charge density of the grid wires.”Ā 

Phew!Ā Quite something, isn’t it? But that’s it really, and it’s actuallyĀ simplerĀ than the ‘direct’ calculations of the field that IĀ googled. Those calculations involve complicated series and logs and what have you, to arrive at the same result: the field away from a grid of charged wires is very nearly uniform.

Let me conclude this post by noting Feynman’s explanation of shielding by a screen. It’s quite terse:

“The method we have just developed can be used to explain why electrostatic shielding by means of a screen is often just as good as with a solid metal sheet. Except within a distance from the screen a few times the spacing of the screen wires, the fields inside a closed screen are zero. We see why copper screen—lighter and cheaper than copper sheet—is often used to shield sensitive electrical equipment from external disturbing fields.”

Hmm… So how does that work?Ā The logic should be similar to the logic I explained when discussing shielding in one of my previous posts. Have a look—if only because it’s a lot easier to understand than the rather convoluted business I presented above. šŸ™‚ But then I guess it’s all par for the course, isn’t it? šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Maxwell, Lorentz, gauges and gauge transformations

Pre-script (dated 26 June 2020): This post got severely mutilated by the removal of material by the dark force. It may, therefore, be difficult to follow the main story-line. :-/

Original post:

I’ve done quite a few posts already on electromagnetism. They were all focused on the math one needs to understand Maxwell’s equations. Maxwell’s equations are a set of (four)Ā differential equations, so they relate some function with its derivatives. To be specific, they relate EĀ and B, i.e. the electric and magnetic field vector respectively, with their derivatives in space and in time. [Let me be explicit here: E and B have three components, but depend on both space as well as time, so we have threeĀ dependent andĀ fourĀ independent variables for each function: E =Ā (Ex,Ā Ey,Ā Ez) = E(x, y, z, t) and B = (Bx, By, Bz) = B(x, y, z, t).] That’s simple enough to understand, but the dynamicsĀ involved are quite complicated, as illustrated below.

Maxwell interactionI now want to do a series on the more interesting stuff, including an exploration of the concept of gaugeĀ in field theory, and I also want to show how one can derive the wave equation for electromagnetic radiation from Maxwell’s equations. Before I start, let’s recall the basic concept of a field.

The reality of fields

I said a couple of time already that (electromagnetic) fields are real. They’re more than just a mathematical structure. Let me show you why. Remember the formula for the electrostatic potential caused by some charge q at the origin:

E 4

We know that the (negative) gradient of this function, at any point in space, gives us the electric field vector at that point: E = ā€“āˆ‡Ī¦. [The minusĀ sign is there because of convention: we take the reference point Φ = 0 at infinity.]Ā Now, the electric field vector gives us the force on a unit charge (i.e. the charge of a proton) at that point. If q is some positive charge, the force will be repulsive, and the unit charge will accelerate away from our q charge at the origin. Hence, energy will be expended, as force over distance implies work is being done: as the charges separate,Ā potentialĀ energy is converted intoĀ kineticĀ energy. Where does the energy come from? The energy conservation law tells us that it must come from somewhere.

It does: the energy comes from the field itself. Bringing in more or bigger charges (from infinity, or just from further away) requires more energy. So the new charges change the field and, therefore, its energy. How exactly?Ā That’s given by Gauss’ Law: the total flux out of a closed surface is equal to:

Gauss Law

You’ll say: flux and energy are two different things. Well… Yes and no. The energy in the field depends on E. Indeed, theĀ formula for the energyĀ densityĀ in space (i.e. the energy per unit volume) is

D 6

Getting the energy over a larger space is just another integral, with the energy density as the integralĀ kernel:

energy integral

Feynman’s illustration below is not very sophisticated but, as usual, enlightening. šŸ™‚

energy in the field

Gauss’ Theorem connects both the math as well as the physics of the situation and, as such, underscores the reality of fields: the energy is not in the electric charges.Ā The energy is in the fields they produce. Everything else is just the principle of superposition of fields – Ā i.e.Ā E = E1Ā + E2 – coming into play. I’ll explain Gauss’ Theorem in a moment. Let me first make some additional remarks.

First, the formulas are valid for electrostatics only (so E and B only vary in space, not in time),Ā so they’re just a piece of the larger puzzle. šŸ™‚Ā As for now, however, note that, if a field is real (or, to be precise, if its energy is real), then the flux is equally real.

Second, let me say something about the units. Field strength (E or, in this case, its normal component EnĀ = EĀ·n) is measured in newton (N) per coulomb (C), so in N/C. The integral above implies that flux is measured in (N/C)Ā·m2. It’s a weird unit because one associates flux with flow and, therefore, one would expect flux is some quantityĀ per unit time and per unit area, so we’d have the m2Ā unit (and the second) in the denominator, not in the numerator. But so that’s true for heat transfer, for mass transfer, for fluid dynamics (e.g. the amount of water flowing through some cross-section) and many other physical phenomena. But for electric flux, it’s different.Ā YouĀ can do a dimensional analysis of the expression above: the sum of the charges is expressed in coulomb (C), and the electric constant (i.e. the vacuum permittivity) is expressed in C2/(NĀ·m2), so, yes, it works: C/[C2/(NĀ·m2)] = (N/C)Ā·m2. To make sense of the units, you should think of the flux as the total flow, and of the field strength as a surface density, so that’s the flux divided by the total area, so (field strength) = (flux)/(area). Conversely, (flux) = (field strength)Ɨ(area). Hence, the unit of flux is [flux] =Ā [field strength]Ɨ[area] = (N/C)Ā·m2.

OK. Now we’re ready forĀ Gauss’ Theorem. šŸ™‚ I’ll also say something about its corollary, Stokes’ Theorem. It’s a bit of a mathematical digression but necessary, I think, for a better understanding of all those operators we’re going to use.

Gauss’ Theorem

The concept of flux is related to the divergenceĀ of a vector field through Gauss’ Theorem. Gauss’s Theorem has nothing to do with Gauss’ Law, except that both are associated with the same genius. Gauss’ Theorem is:

Gauss Theorem

The āˆ‡Ā·CĀ in the integral on the right-hand side is theĀ divergenceĀ of a vector field. It’s the volume density of the outward flux of a vector fieldĀ from an infinitesimal volume around a given point.

Huh?Ā What’s a volume density? Good question. Just substitute C for E in the surface and volume integral above (the integral on the left is a surface integral, and the one on the right is a volume integral), and think about the meaning of what’s written. To help you, let me also include the concept of linearĀ density, so we have (1)Ā linear, (2) surface and (3) volume density. Look at that representation of a vector field once again: we said the density of lines represented the magnitude of E. But what density? The representation hereunder is flat, so we can think of a linear density indeed, measured along the blue line: so the flux would be six (that’s the number of lines), and the linear density (i.e. the field strength) is six divided by the length of the blue line.

Linear density

However, we defined field strength as a surface density above, so that’s the flux (i.e. the number of field lines) divided by the surface area (i.e. the area of a cross-section): think of the square of the blue line, and field lines going through that square. That’s simple enough. But what’s volume density? How do we count the number of lines insideĀ of a box? The answer is: mathematicians actually define itĀ for an infinitesimally small cube by adding the fluxes out of the six individual faces of an infinitesimally small cube:

Volume density for small cube 1

So, the truth is: volume density is actually defined as a surfaceĀ density, but for an infinitesimally small volume element.Ā That, in turn, gives us the meaning of theĀ divergenceĀ of a vector field. Indeed, the sum of the derivatives above is just āˆ‡Ā·CĀ (i.e. the divergence of C), and Ī”xĪ”yĪ”z is the volume of our infinitesimal cube, so the divergence of some field vector C at some point P is the flux – i.e. the outgoing ‘flow’ of C – per unit volume, in the neighborhood of P, as evidenced by writing

Volume density for small cube

Indeed, just bringĀ Ī”V to the other side of the equation to check the ‘per unit volume’ aspect of what I wrote above. The whole idea is to determine whether the small volume is like a sink or like a source, and to what extent. Think of the field near a point charge, as illustrated below. Look at the black lines: they are the field lines (the dashed lines are equipotential lines) and note how the positive charge is a source of flux, obviously, while the negative charge is a sink.

equipotential

Now, the next step is to acknowledge that the total flux from a volume is the sum of the fluxes out of each part. Indeed, the flux through the part of the surfaces common to two parts will cancel each other out. Feynman illustrates that with a rough drawing (below) and I’ll refer you to hisĀ LectureĀ on it for more detail.

cut

So… Combining all of the gymnastics above – and integrating the divergence over an entire volume, indeed – Ā we get Gauss’ Theorem:

Gauss Theorem

Stokes’ Theorem

There is a similar theorem involving the circulationĀ of a vector, rather than its flux. It’s referred to as Stokes’ Theorem. Let me jot it down:

Stokes Theorem

We have aĀ contourĀ integral here (left) and a surface integral (right). The reasoning behind is quite similar: a surface bounded by some loopĀ Ī“ is divided into infinitesimally small squares, and the circulation aroundĀ Ī“ is the sum of the circulations around the little loops. We should take care though: the surface integral takes theĀ normalĀ component of āˆ‡Ć—C, so that’s (āˆ‡Ć—C)nĀ = (āˆ‡Ć—C)Ā·n. The illustrations below should help you to understand what’s going on.

Stokes Theorem 1Stokes Theorem 2

The electric versus the magnetic force

There’s more than just the electric force: we also have the magnetic force. The so-called LorentzĀ force is the combination of both. The formula, for some charge q in an electromagnetic field, is equal to:

Lorentz force

Hence, if the velocity vectorĀ vĀ is not equal to zero, we need to look at the magnetic field vectorĀ B too!Ā The simplest situation is magnetostatics, so let’s first have a look at that.

Magnetostatics imply that that the flux of E doesn’t change, so Maxwell’s third equation reduces to c2āˆ‡Ć—BĀ = j/ε0. So we just have a steadyĀ electric current (j): noĀ accelerating charges. Maxwell’s fourth equation, āˆ‡ā€¢BĀ = 0, remains what is was: there’s no such thing as a magnetic charge. The Lorentz force also remains what it is, of course: F = q(E+vƗB) = qE +qvƗB. Also note that the v, j and the lack of a magnetic charge all point to the same: magnetism is just a relativistic effect of electricity.

What about units? Well… While the unit of E, i.e. the electric field strength, is pretty obvious from theĀ F = qEĀ term  – hence, E = F/q, and so the unit of E must be [force]/[charge] = N/C – the unit of the magnetic field strength is more complicated. Indeed, the F =Ā qvƗBĀ identity tells us it must be (NĀ·s)/(mĀ·C), because 1 N = 1CĀ·(m/s)Ā·(NĀ·s)/(mĀ·C). Phew!Ā That’s as horrendous as it looks, and that’s why it’s usually expressed using its shorthand, i.e. the tesla: 1 T = 1 (NĀ·s)/(mĀ·C).Ā Magnetic flux is the same concept as electric flux, so it’sĀ (field strength)Ɨ(area). However, now we’re talkingĀ magneticĀ field strength, so its unit is TĀ·m2Ā =Ā (NĀ·sĀ·m2Ā )/(mĀ·C) =Ā (NĀ·sĀ·m)/C, which is referred to as the weberĀ (Wb). Remembering thatĀ 1 volt = 1 NĀ·m/C, it’s easy to see that a weber is also equal to 1Ā Wb = 1 VĀ·s. In any case, it’s a unit that is not soĀ easy to interpret.

Magnetostatics is a bit of a weird situation. It assumes steady fields, so theĀ āˆ‚E/āˆ‚t and āˆ‚B/āˆ‚t terms in Maxwell’s equations can be dropped. In fact, c2āˆ‡Ć—BĀ = j/ε0Ā implies that āˆ‡Ā·(c2āˆ‡Ć—BĀ )Ā =Ā āˆ‡Ā·(j/ε0) and, therefore, that āˆ‡Ā·jĀ = 0. Now, āˆ‡Ā·jĀ = ā€“āˆ‚Ļ/āˆ‚t and, therefore, magnetostatics is a situation which assumes āˆ‚Ļ/āˆ‚t = 0. So we have electric currents butĀ no change in charge densities. To put it simply, we’re not lookingĀ at a condenser that is charging or discharging, although that condenser may act like the battery or generator that keeps the charges flowing! But let’s go along with the magnetostatics assumption. What can we say about it? Well… First, we have the equivalent of Gauss’ Law, i.e. AmpĆØre’s Law:

Ampere Law

We have a line integral here around a closed curve, instead of a surface integral over a closed surface (Gauss’ Law), but it’s pretty similar: instead of the sum of the charges inside the volume, we have the current through the loop, and then an extra c2Ā factor in the denominator, of course. Combined with the āˆ‡ā€¢BĀ = 0 equation, this equation allows us to solve practical problems. But I am not interested in practical problems. What’s the theory behind?

The magnetic vector potential

The āˆ‡ā€¢BĀ = 0 equation is true, always, unlike theĀ āˆ‡Ć—EĀ = 0 expression, which is true for electrostatics only (no moving charges). It says the divergenceĀ of B is zero,Ā always, and, hence, it means we can represent B as the curl of another vector field, always. That vector field is referred to as the magneticĀ vectorĀ potential, and we write:

āˆ‡Ā·B = āˆ‡Ā·(āˆ‡Ć—A) = 0 and, hence, B =Ā āˆ‡Ć—A

In electrostatics, we had the other theorem: if the curl of a vector field is zero (everywhere), then the vector field can be represented as the gradient of some scalar function, so if āˆ‡Ć—CĀ = 0, then there is some ĪØĀ for which C =Ā āˆ‡ĪØ. Substituting C forĀ E, and taking into account our conventions on charge and the direction of flow, we get E = ā€“āˆ‡Ī¦. Substituting E in Maxwell’s first equation (āˆ‡ā€¢E = ρ/ε0) then gave us the so-calledĀ PoissonĀ equation: āˆ‡2Φ = ρ/ε0, which sums up the whole subject of electrostatics really! It’s all in there!

Except magnetostatics, of course. Using the (magnetic)Ā vector potentialĀ A, all of magnetostatics is reduced to another expression:

āˆ‡2A=Ā āˆ’j/ε0, with āˆ‡Ā·A = 0

Note the qualifier: āˆ‡Ā·A = 0. Why should the divergence of A be equal to zero? You’re right. It doesn’t have to be that way. We know that āˆ‡Ā·(āˆ‡Ć—C) = 0, for any vector field C, andĀ alwaysĀ (it’s a mathematical identity, in fact, so it’s got nothing to do with physics), but choosing A such that āˆ‡Ā·A = 0 is just a choice. In fact, as I’ll explain in a moment, it’s referred to as choosing aĀ gauge.Ā The āˆ‡Ā·A = 0 choice is a very convenient choice, however, as it simplifies our equations. Indeed,Ā c2āˆ‡Ć—BĀ = j/ε0Ā = c2āˆ‡Ć—(āˆ‡Ć—A), and – from our vector calculus classes – we know that āˆ‡Ć—(āˆ‡Ć—C) = āˆ‡(āˆ‡Ā·C) – āˆ‡2C. Combining that with our choice of AĀ (which is such thatĀ āˆ‡Ā·A = 0, indeed), we get the āˆ‡2A=Ā āˆ’j/ε0 expression indeed, which sums up the whole subject of magnetostatics!

The point is: if the time derivatives in Maxwell’s equations, i.e. āˆ‚E/āˆ‚t and āˆ‚B/āˆ‚t, are zero, then Maxwell’s four equations can be nicely separated into two pairs: the electric and magnetic field are not interconnected. Hence, as long as charges and currents are static, electricity and magnetism appear as distinct phenomena, and the interdependence of E and B does not appear. So we re-write Maxwell’s set of four equations as:

  1. Electrostatics:Ā āˆ‡ā€¢E = ρ/ε0Ā and āˆ‡Ć—E = 0
  2. Magnetostatics: āˆ‡Ć—BĀ = j/c2ε0Ā and āˆ‡ā€¢B = 0

Note that electrostatics is a neat example of a vector field with zero curl and a given divergence (ρ/ε0), while magnetostatics is a neat example of a vector field with zero divergence and a given curl (j/c2ε0).

Electrodynamics

But reality is usually not so simple. WithĀ time-varyingĀ fields, Maxwell’s equations are what they are, and so thereĀ isĀ interdependence, as illustrated in the introduction of this post. Note, however, that the magnetic field remainsĀ divergence-freeĀ in dynamics too! That’s because there is no such thing as a magnetic charge: we only have electric charges. SoĀ āˆ‡Ā·B = 0 and we can define a magneticĀ vectorĀ potentialĀ AĀ and re-write B as B =Ā āˆ‡Ć—A, indeed.

I am writing a vector potential field because, as I mentioned a couple of times already, we can choose A. Indeed, as long asĀ āˆ‡Ā·A = 0, it’s fine, so we can add curl-free components to the magnetic potential: it won’t make a difference. This condition is referred to as gauge invariance. I’ll come back to that, and also show why this is what it is.

While we can easily get B from A because of the B =Ā āˆ‡Ć—A, getting E from some potential is a different matter altogether. It turns out we can get E using the following expression, which involves both Φ (i.e. the electric or electrostatic potential) as well as A (i.e. the magnetic vector potential):

E = ā€“āˆ‡Ī¦ – āˆ‚A/āˆ‚t

Likewise, one can show that Maxwell’s equations can be re-written in terms of Φ andĀ A, rather than in terms of E and B. The expression looks rather formidable, but don’t panic:

Equations 2

Just look at it. We have two ‘variables’ here (Φ andĀ A) and two equations, so the system is fully defined. [Of course, the second equation is three equations really: one for each component x, y and z.]Ā What’s the point? Why would we want to re-write Maxwell’s equations? The first equation makes it clear that theĀ scalar potential (i.e. the electric potential) is a time-varying quantity, so things are not, somehow, simpler. The answer is twofold. First, re-writing Maxwell’s equations in terms of the scalar and vector potential makes sense because we have (fairly) easy expressions for their valueĀ in time and in space as a function of the charges and currents. For statics, these expressions are:

Integrals staticsSo it is, effectively, easier to first calculate the scalar and vector potential, and then get E and B from them. ForĀ dynamics, the expressions are similar:

Integrals dynamics

Indeed, they are likeĀ the integrals for statics, butĀ with “aĀ small and physically appealing modification”, as Feynman notes: when doing the integrals, we must use the so-called retarded timeĀ t′ = t āˆ’ r12/ct’. The illustration below shows how it works: the influences propagate from point (2) to point (1) at the speedĀ c, so we must use the values of ρ andĀ j at theĀ timeĀ t′ = t āˆ’ r12/ct’Ā indeed!

Retarded timeThe second aspect of the answer to the question of why we’d be interested in Φ and A has to do with the topic I wanted to write about here: the concept of aĀ gaugeĀ and aĀ gauge transformation.

Gauges and gauge transformations in electromagnetics

Let’s see what we’re doing really. We calculate some AĀ and then solve for B by writing: B = āˆ‡Ć—A. Now, I say someĀ A because any A‘ = A +Ā āˆ‡ĪØ, with ĪØĀ any scalar field really. Why? Because the curlĀ of the gradient ofĀ ĪØ – i.e. curl(gradĪØ) = āˆ‡Ć—(āˆ‡ĪØ) – is equal to 0. Hence, āˆ‡Ć—(A +Ā āˆ‡ĪØ) =Ā āˆ‡Ć—A +Ā āˆ‡Ć—āˆ‡ĪØ =Ā āˆ‡Ć—A.

So we have B, and now we need E. So the next step is to take Faraday’s Law, which is Maxwell’s second equation:Ā āˆ‡Ć—E =Ā ā€“āˆ‚B/āˆ‚t. Why this one? It’s a simple one, as it does not involve currents or charges. So we combine this equation and ourĀ B = āˆ‡Ć—AĀ expression and write:

āˆ‡Ć—E =Ā ā€“āˆ‚(āˆ‡Ć—A)/āˆ‚t

Now, these operators are tricky but you can verify this can be re-written as:

āˆ‡Ć—(EĀ + āˆ‚A/āˆ‚t) = 0

Looking carefully, we see this expression says that EĀ + āˆ‚A/āˆ‚t is some vector whose curl is equal to zero. Hence, this vector must be the gradient ofĀ something. When doing electrostatics,Ā When we worked on electrostatics, we only had E, not the āˆ‚A/āˆ‚t bit, and we said that E tout courtĀ was the gradient of something, so we wrote E = āˆ’āˆ‡Ī¦. We now do the same thing forĀ EĀ + āˆ‚A/āˆ‚t, so we write:

EĀ + āˆ‚A/āˆ‚t = āˆ’āˆ‡Ī¦

So we use the same symbol Φ but it’s a bit of a different animal, obviously. However, it’s easy to see that, if the āˆ‚A/āˆ‚t would disappear (as it does in electrostatics, where nothing changes with time), we’d get our ‘old’ āˆ’āˆ‡Ī¦. Now, EĀ + āˆ‚A/āˆ‚t = āˆ’āˆ‡Ī¦ can be written as:

EĀ = āˆ’āˆ‡Ī¦Ā ā€“Ā āˆ‚A/āˆ‚t

So, what’s the big deal? We wrote B and E as a function of Φ and A. Well, we said we could replace A by anyĀ A‘ = A +Ā āˆ‡ĪØ but, obviously, such substitution would not yield the sameĀ E. To get the same E, we need some substitution rule for Φ as well. Now, you can verify we will get the same E if we’d substitute Φ for Φ’ = Ī¦Ā ā€“Ā āˆ‚ĪØ/āˆ‚t. You should check it by writing it all out:

EĀ = āˆ’āˆ‡Ī¦’ā€“āˆ‚A’/āˆ‚t = āˆ’āˆ‡(Ī¦ā€“āˆ‚ĪØ/āˆ‚t)ā€“āˆ‚(A+āˆ‡ĪØ)/āˆ‚t

= āˆ’āˆ‡Ī¦+āˆ‡(āˆ‚ĪØ/āˆ‚t)ā€“āˆ‚A/āˆ‚tā€“āˆ‚(āˆ‡ĪØ)/āˆ‚t =Ā āˆ’āˆ‡Ī¦Ā ā€“Ā āˆ‚A/āˆ‚t =Ā E

Again, the operators are a bit tricky, but the +āˆ‡(āˆ‚ĪØ/āˆ‚t) andĀ ā€“āˆ‚(āˆ‡ĪØ)/āˆ‚t terms do cancel out. Where are we heading to? When everything is said and done, we do need to relate it all to the currents and the charges, because that’s the real stuff out there. So let’s take Maxwell’s āˆ‡ā€¢E = ρ/ε0Ā equation, which has the charges in it, and let’s substitute E forĀ EĀ = āˆ’āˆ‡Ī¦Ā ā€“Ā āˆ‚A/āˆ‚t. We get:

Capture

That equation can be re-written as:

equation 1

So we have one equation here relating Φ and A to the sources. We need another one, and we also need to separate Φ and A somehow. How do we do that?

Maxwell’s fourth equation, i.e. c2āˆ‡Ć—BĀ = j/ε0Ā +Ā āˆ‚E/āˆ‚t can, obviously, be written asĀ c2āˆ‡Ć—BĀ āˆ’Ā āˆ‚E/āˆ‚t = j/ε0. Substituting both E and B yields the following monstrosity:

equation 3

We can now apply the generalĀ āˆ‡Ć—(āˆ‡Ć—C) = āˆ‡(āˆ‡Ā·C) – āˆ‡2CĀ identity to the first term to get:

equation 4

It’s equally monstrous, obviously, but we can simplify the whole thing by choosing Φ and A in a clever way. For the magnetostatic case, we chose A such that āˆ‡Ā·A = 0. We could have chosen something else. Indeed, it’s not because B is divergence-free, that A has to be divergence-free too! For example, I’ll leave it to you to show that choosing āˆ‡Ā·A such that

equation 5also respects the general condition that any A and Φ we choose must respect theĀ A‘ = A +Ā āˆ‡ĪØ and Φ’ = Ī¦Ā ā€“Ā āˆ‚ĪØ/āˆ‚t equalities. Now, if we chooseĀ āˆ‡Ā·A such thatĀ āˆ‡Ā·A =Ā āˆ’c–2Ā·āˆ‚Ī¦/āˆ‚t indeed, then the two middle terms in our monstrosity cancel out, and we’re left with a much simpler equation for A:

equation 6

In addition, doing the substitution in our other equation relating Φ and A to the sources yields an equation for Φ that has the same form:

equation 7

What’s the big deal here? Well… Let’s write it all out. The equation above becomes:

wave equation

That’s a wave equation in three dimensions. In case you wonder, just check one of my posts on wave equations. The one-dimensional equivalent for a wave propagating in the x direction at speed c (like a sound wave, for example)Ā isĀ āˆ‚2Φ/āˆ‚x2Ā =Ā c–2Ā·āˆ‚2Φ/āˆ‚t2, indeed. The equation for A yields above yields similar wave functions for A‘s components Ax, Ay, andĀ Az.

So, yes, it isĀ a big deal. We’ve written Maxwell’s equations in terms of the scalar (Φ) and vector (A) potential and in a form that makes immediately apparent that we’re talking electromagnetic waves moving out at the speed c. Let me copy them again:

Equations 2

You may, of course, say that you’d rather have a wave equation for E and B, rather than for A and Φ. Well… That can be done. Feynman gives us two derivations that do so. The first derivation is relativelyĀ simple and assumes theĀ sourceĀ our electromagnetic wave moves in one direction only. The second derivation is much more complicated and gives an equation for E that, if you’ve read the first volume of Feynman’sĀ Lectures, you’ll surely remember:

equation for E

The links are there, and so I’ll let you have fun with those LecturesĀ yourself. I am finished here, indeed, in terms of what I wanted to do in this post, and that is to say a few words about gauges in field theory. It’s nothing much, really, and so we’ll surely have to discuss the topic again, but at least you now know what a gauge actually is in classical electromagnetic theory. Let’s quickly go over the concepts:

  1. Choosing the āˆ‡Ā·A is choosing a gauge, or a gauge potentialĀ (because we’re talking scalar and vector potential here).Ā The particular choice is also referred to asĀ gauge fixing.
  2. Changing A by adding āˆ‡Ļˆ is called a gauge transformation, and the scalar functionĀ ĪØ is referred to as aĀ gauge function.Ā The fact thatĀ we can add curl-free components to the magnetic potential without them making any difference is referred to as gauge invariance.
  3. Finally, the āˆ‡Ā·A =Ā āˆ’c–2Ā·āˆ‚Ī¦/āˆ‚t gauge is referred to as a Lorentz gauge.

Just to make sure you understand: why is thatĀ Lorentz gauge so special? Well… Look at the whole argument once more: isn’t it amazing we get such beautiful (wave) equations if we stick it in? Also look at the functional shape of the gauge itself: it looks like a wave equation itself! […] Well… No… It doesn’t. I am a bit too enthusiastic here. We do have the sameĀ 1/c2Ā and a time derivative, but it’s not a wave equation.Ā šŸ™‚ In any case, it allĀ confirms, once again, that physics is all about beautiful mathematical structures. But, again, it’s not math only. There’s something realĀ out there. In this case, that ‘something’ is a traveling electromagnetic field. šŸ™‚

But why do we call it a gauge? That should be equally obvious. It’s really like choosing a gauge in another context, such as measuring the pressure of a tyre, as shown below. šŸ™‚

abs-gauge-press

Gauges and group theory

You’ll usually see gauges mentioned with some reference to group theory. For example, you will see or hear phrases like: “The existence of arbitrary numbers of gauge functions ψ(r, t) corresponds to the U(1) gauge freedom of the electromagnetic theory.” The U(1) notation stands for aĀ unitary group of degree n = 1. It is also known as theĀ circle group.Ā Let me copy the introduction to the unitary group from the Wikipedia article on it:

In mathematics, the unitary group of degree n, denoted U(n), is the groupĀ of n Ɨ n unitary matrices, with the group operation that of matrix multiplication. The unitary group is a subgroup of the general linear group GL(n, C).Ā In the simple case n = 1, the group U(1) corresponds to the circle group, consisting of all complex numbers with absolute value 1 under multiplication. All the unitary groups contain copies of this group.

The unitary group U(n) is a real Lie group of of dimension n2. The Lie algebra of U(n) consists of n Ɨ n skew-Hermitian matrices, with the Lie bracket given by the commutator.Ā The general unitary group (also called the group of unitary similitudes) consists of all matrices A such that A*A is a nonzero multiple of the identity matrix, and is just the product of the unitary group with the group of all positive multiples of the identity matrix.

Phew!Ā Does this make you any wiser? If anything, it makes me realize I’ve still got a long way to go. šŸ™‚ The Wikipedia article on gauge fixingĀ notes something that’s more interesting (if only because I more or less understand what it says):

Although classical electromagnetism is now often spoken of as a gauge theory, it was not originally conceived in these terms. The motion of a classical point charge is affected only by the electric and magnetic field strengths at that point, and the potentials can be treated as a mere mathematical device for simplifying some proofs and calculations. Not until the advent of quantum field theory could it be said that the potentials themselves are part of the physical configuration of a system. The earliest consequence to be accurately predicted and experimentally verified was the Aharonov–Bohm effect, which has no classical counterpart.

This confirms, once again, that the fields are real. In fact, what this says is that theĀ potentialsĀ are real: they have a meaningful physical interpretation. I’ll leave it to you to expore that Aharanov-Bohm effect. In the meanwhile, I’ll study what Feynman writes on potentials and all that as used in quantum physics. It will probably take a while before I’ll get into group theory though. :-/

Indeed, it’s probably best to study physics at a somewhat less abstract level first, before getting into the more sophisticated stuff.

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 20, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Music and Math

Pre-scriptum (dated 26 June 2020): These posts on elementary math and physics have not suffered much the attack by the dark force—which is good because I still like them. While my views on the true nature of light, matter and the force or forces that act on them have evolved significantly as part of my explorations of a more realist (classical) explanation of quantum mechanics, I think most (if not all) of the analysis in this post remains valid and fun to read. In fact, I find the simplest stuff is often the best. šŸ™‚

Original post:

I ended my previous post, on Music and Physics, by emphatically making the point that music is all about structure, about mathematical relations. Let me summarize the basics:

1. The octave is the musical unit, defined as the interval between two pitches with the higher frequency being twiceĀ the frequency of the lowerĀ pitch. Let’sĀ denote the lower and higher pitch byĀ a and b respectively, so we say that b‘s frequency is twiceĀ that of a.

2. We then divide the [a, b] interval (whose length is unity) in twelve equal sub-intervals, which define eleven notes in-between a and b. The pitch of the notes in-between is defined by the exponential function connecting a and b. What exponential function? The exponential function with base 2, so that’s the function y =Ā 2x.

Why base 2? Because of the doubling of the frequencies when going from a to b, and when going from b to b + 1, and from b + 1 to b + 2, etcetera. In music, we give a, b, b + 1, b + 2, etcetera the sameĀ name, or symbol: A, for example. Or Do. Or C. OrĀ Re. Whatever. If we have the unit and the number of sub-intervals, all the rest follows. We just add a number to distinguish the various As, or Cs, or Gs, so we write A1, A2, etcetera. Or C1, C2, etcetera. The graph below illustrates the principle for the interval between C4 and C5. Don’t think the function is linear. It’s exponential: note the logarithmic frequency scale. To make the point, I also inserted another illustration (credit for that graph goes to another blogger).

Frequency_vs_name

equal-tempered-scale-graph-linear

You’ll wonder: why twelve sub-intervals? Well… That’s random. Non-Western cultures use a different number. Eight instead of twelve, for example—which is more logical, at first sight at least:Ā eight intervals amounts to dividing the interval in two equal halves, and the halves in halves again, and then once more: so the length of the sub-interval is then 1/2Ā·1/2Ā·1/2 = (1/2)3Ā = 1/8. But why wouldn’t we divide by three, so we have 9 = 3Ā·3 sub-intervals? Or by 27 = 3Ā·3Ā·3? Or by 16? Or by 5?

The answer is: we don’t know. The limited sensitivity of our ear demands that the intervals be cut up somehow. [You can do tests of the sensitivity of your ear to relative frequency differences online: it’s fun. Just try them! Some of the sites may recommend a hearing aid, but don’t take that crap.] So… The bottom line is that,Ā somehow, mankind settled on twelve sub-intervals within our musical unit—or our sound unit, I should say.Ā So it is what it is, and the ratio of the frequencies between two successive (semi)tones (e.g. C and C#, or E and F, as E and F are also separated by one half-step only)Ā is 21/12Ā = 1.059463… Hence, the pitch of each note is about 6% higher than the pitch of the previous note. OK. Next thing.

3.Ā What’s the similarity between C1, C2, C3 etcetera? Or between A1, A2, A3 etcetera? The answer is: harmonics. The frequency of the first overtoneĀ of a string tuned at pitch A3 (i.e. 220 Hz) is equal to the fundamental frequency of a string tuned at pitch A4 (i.e. 440 Hz). Likewise,Ā the frequency of the (pitch of the) C4 note above (which is the so-called middle C)Ā is 261.626 Hz, while the frequency of the (pitch of the) next C note (C5) is twiceĀ that frequency: 523.251 Hz.Ā [I should quickly clarify the terminology here: a tone consists of several harmonics, with frequencies f, 2Ā·f, 3Ā·f,… nĀ·f,… The first harmonic is referred to as the fundamental, with frequencyĀ f. The second, third, etc harmonics are referred to asĀ overtones, with frequency 2Ā·f, 3Ā·f, etc.]

To make a long story short: our ear is able to identify the individual harmonics in a tone, and if the frequency of the first harmonic of one tone (i.e. the fundamental) is the same frequency as the second harmonic of another, then we feel they are separated by one musical unit.

Isn’t that most remarkable? Why would it be that way?

My intuition tells me I should look at the energy of the components. The energy theorem tells us that the total energy in a wave is just the sum of the energies in all of the Fourier components. Surely, the fundamental must carry most of the energy, and then the first overtone, and then the second. Really? Is that so?

Well… I checked online to see if there’s anything on that, but my quick check reveals there’s nothing much out there in terms of research: if you’dĀ googleĀ ‘energy levels of overtones’, you’ll get hundreds of links to research on the vibrational modes of molecules, but nothing that’s related to music theory.Ā So… Well… Perhaps this is my first truly original post! šŸ™‚ Let’s go for it. šŸ™‚

The energy in a wave is proportional to the square of its amplitude, and we must integrate over one period (T) of the oscillation. The illustration below should help you to understand what’s going on. The fundamental mode of the wave is an oscillation with a wavelength (Ī»1) that is twiceĀ the length of the string (L). For the second mode, the wavelength (Ī»2) is just L. For the third mode, we find that Ī»3Ā = (2/3)Ā·L. More in general, the wavelength of the nthĀ mode isĀ Ī»nĀ = (2/n)Ā·L.

modes

The illustration above shows that we’re talking sine waves here, differing in their frequency (or wavelength) only. [The speed of the wave (c), as it travels back and forth along the string, i constant, so frequency and wavelength are in that simple relationship: c = fĀ·Ī».] Simplifying and normalizing (i.e. choosing the ‘right’ units by multiplying scales with some proportionality constant), the energy of the first mode would be (proportional to):

Integral 1

What about the second and third modes? For the second mode, we have two oscillations per cycle, but we still need to integrate over the period of the first mode T = T1,Ā which isĀ twiceĀ the period of the second mode: T1Ā = 2Ā·T2. Hence,Ā T2Ā = (1/2)Ā·T1. Therefore, the argument of the sine wave (i.e. theĀ x variable in the integral above) should go from 0 to 4Ļ€. However, we want to compare the energies of the various modes, so let’s substitute cleverly. We write:

Integral 2

The period of the third mode is equal to T3Ā = (1/3)Ā·T1. Conversely, T1Ā = 3Ā·T3. Hence, the argument of the sine wave should go from 0 to 6Ļ€. Again, we’ll substitute cleverly so as to make the energies comparable. We write:

Integral 3

NowĀ thatĀ is interesting! For a so-called idealĀ string, whose motion is the sum of a sinusoidal oscillation at the fundamental frequency f, another at the second harmonic frequency 2Ā·f, another at the third harmonic 3Ā·f, etcetera, we find that the energies of the various modes are proportional to the values in the harmonic series 1, 1/2, 1/3, 1/4,… 1/n, etcetera. Again, Pythagoras’ conclusion was wrong (the ratio of frequencies of individual notes do not respect simple ratios), but his intuition was right: the harmonic series āˆ‘nāˆ’1Ā (n = 1, 2,…,āˆž) is veryĀ relevant in describing natural phenomena. It gives us the respective energies of the various naturalĀ modesĀ of a vibrating string! In the graph below, the values are represented asĀ areas. It is all quite deep and mysterious really!

602px-Integral_Test

So now we know why we feel C4 and C5 have so much in common that we call them by the same name: C, orĀ Do. It also helps us to understand why the E and A tones have so much in common:Ā theĀ third harmonic of the 110 Hz A2Ā string corresponds to the fundamental frequency of the E4 string: both are 330 Hz! Hence, E and A have ‘energy in common’, so to speak, but less ‘energy in common’ than two successive E notes, or two successive A notes, or two successive C notes (like C4 and C5).

[…]Ā Well… Sort of… In fact, the analysis above is quite appealing but – I hate to say it – it’s wrong, as I explain in myĀ post scriptumĀ to this post. It’s like Pythagoras’ number theory of the Universe: the intuition behind is OK, but the conclusions aren’t quite right. šŸ™‚

Ideality versus reality

We’ve been talking idealĀ strings. Actual tones coming out of actual strings have a quality, which is determined by the relative amounts of the various harmonics that are present in the tone, which is notĀ some simple sum of sinusoidal functions. Actual tones have a waveform that may resemble something like the wavefunction I presented in my previous post, when discussing Fourier analysis. Let me insert that illustration once again (and let me also acknowledge its source once more: it’sĀ Wikipedia). The red waveformĀ is the sum of six sine functions, with harmonically related frequencies, but with different amplitudes. Hence, the energy levels of the various modes will not be proportional to the values in that harmonic seriesĀ āˆ‘nāˆ’1, with n = 1, 2,…,āˆž.

Fourier_series_and_transform

Das wohltemperierte Klavier

Nothing in what I wrote above is related to questions of taste like: why do I seldomly select a classical music channel on my online radio station? Or why am I not into hip hop, even if my taste for music is quite similar to that of the common crowd (as evidenced from the fact that I like ‘Listeners’ Top’ hit lists)?

Not sure. It’s an unresolved topic, I guess—involvingĀ rhythmĀ and other ‘structures’ I didĀ notĀ mention.Ā Indeed, all of the above just tells us a nice story about the structure of theĀ languageĀ of music: it’s a story about the tones, and how they are related to each other. That relation is, in essence, an exponential function with base 2. That’s all. Nothing more, nothing less. It’s remarkably simple and, at the same time, endlessly deep. šŸ™‚ But so it isĀ notĀ a story about the structure of a musical piece itself, of a pop song of Ellie Goulding, for instance, or one of Bach’s preludesĀ orĀ fugues.

That brings me back to the original question I raised in my previous post. It’s a question which was triggered, long time ago, when I tried to read Douglas Hofstadter‘sĀ Gƶdel, Escher and Bach, frustrated because my brother seemed to understand it, and I didn’t. So I put it down, and never ever looked at it again. So what is it really about that famous piece of Bach?

Frankly, I still amn’t sure. As I mentioned in my previous post, musicians were struggling to find a tuning system that would allow them to easily transpose musical compositions.Ā Transposing music amounts to changing the so-calledĀ keyĀ of a musical piece, so that’s moving the whole piece up or down in pitch by some constant interval that is not equal to anĀ octave. It’s a piece of cake now. In fact, increasing or decreasing the playback speed of a recording also amounts to transposing a piece: a increase or decrease of the playback speed by 6% will shift the pitch up or down by about one semitone. Why? Well… Go back to what I wrote above about that 12th root of 2. We’ve got the right tuning system now, and so everything is easy. Logarithms are great! šŸ™‚

Back to Bach. Despite their admiration for the Greek ideas around aesthetics – and,Ā most notably, their fascination with harmonic ratios! – (almost) all RenaissanceĀ musicians were struggling with the so-calledĀ PythagoreanĀ tuning system, which was used until the 18th century and which was based on aĀ correctĀ observation (similar strings, under the same tension but differing in length, sound ā€˜pleasant’ when sounded togetherĀ if – and only if  – the ratio of the length of the strings is like 1:2, 2:3, 3:4, 3:5, 4:5, etcetera) but aĀ wrong conclusionĀ (the frequencies of musical tones should also obey the same harmonic ratios), and Bach’s so-calledĀ ‘good’Ā temperament tuning system was designed such that the piece could, indeed, be played in most keys without sounding… well… out of tune. šŸ™‚

Having said that, the modern ‘equal temperament’ tuning system, which prescribes that tuning should be done such that the notes are in the above-described simpleĀ logarithmic relation to each other, had already been invented. So the true question is: why didn’t Bach embrace it? Why did he stick to ratios? Why did it take so long for the right system to be accepted?

I don’t know. If youĀ google, you’ll find a zillion of possible explanations. As far as I can see, most are all rather mystic. More importantly, most of them do not mention many facts. My explanation is rather simple: while Bach was, obviously, a musical genius, he may not have understood what an exponential, or a logarithm, is all about. Indeed, a quick read of summary biographies reveals thatĀ Bach studied a wide range of topics, like Latin and Greek, and theology—of course! But math is not mentioned. He didn’t write about tuning and all that: all of his time went to writing musical masterpieces!

What the biographies do mention is that he always found other people’s tunings unsatisfactory, and that he tuned hisĀ harpsichords and clavichords himself. Now thatĀ is quite revealing, I’d say! In my view, Bach couldn’t care less about the ratios. He knew something was wrong with the Pythagorean system (or the variants as were then used, which are referred to as meantone temperament)Ā and, as a musical genius, he probably ended up tuningĀ by ear.Ā [For those who’d wonder what I am talking about, let me quickly insert a Wikipedia graph illustrating the difference between the Pythagorean system (and two of these meantoneĀ variants) and theĀ equal temperamentĀ tuning system in use today.]

Meantone

So… What’s the point I am trying to make? Well… Frankly, I’d bet Bach’s own tuning wasĀ actually equal temperament, and so he should have named his masterpieceĀ Das gleichtemperierte Klavier. Then we wouldn’t have all that ‘noise’ around it. šŸ™‚

Post scriptum: Did you like the argument on the respective energy levels of the harmonics of an ideal string? Too bad. It’s wrong. I made a common mistake: when substituting variables in the integral, I ‘forgot’ to substitute the lower and upper bound of the interval over which I was integrating the function. The calculation below corrects the mistake, and so it does the required substitutions—for the first three modes at least. What’s going on here? Well… Nothing much…Ā I just integrate over the length L taking a snapshot at t = 0 (as mentioned, we can always shift the origin of our independent variable, so here we do it for time and so it’s OK). Hence, the argument of our wave function sin(kxāˆ’Ļ‰t) reduces to kx, with k = 2Ļ€/Ī», and λ = 2L, λ = L, λ = (2/3)Ā·L for the first, second and third mode respectively. [As for solving the integral of the sine squared, you canĀ googleĀ the formula, and please do check my substitutions. They should be OK, but… Well… We never know, do we? :-)]

energy integrals

[…] No… This doesn’t make all that much sense either. Those integrals yieldĀ the same energy for all three modes. Something must be wrong: shorter wavelengths (i.e. higher frequencies) are associated with higher energy levels. Full stop. So the ‘solution’ above can’t be right… […] You’re right. That’s where the time aspect comes into play. We were taking a snapshot, indeed, and the mean value of the sine squared function is 1/2 = 0.5, as should be clear from Pythagoras’ theorem: cos2x + sin2x = 1. So what I was doing is like integrating a constant function over the same-length interval. So… Well… Yes: no wonder I get the same value again and again.

[…]

We need to integrate over the sameĀ time interval. You could do that, as an exercise, but there’s a more direct approach to it: the energy of a wave is directly proportional to its frequency, so we write: E ∼ f. If the frequency doubles, triples, quadruples etcetera, then its energy doubles, triples, quadruples etcetera too. But – remember – we’re talking one string only here, with a fixed wave speedĀ c = λ·f – so f = c/Ī» (read: the frequency is inversely proportional to the wavelength) – and, therefore (assuming the same (maximum) amplitude), we get that the energy level of each mode is inversely proportional to the wavelength, so we find that E ∼ 1/f.

Now, with direct or inverse proportionality relations, we can always invent some new unit that makes the relationship an identity, so let’s do that and turn it into an equation indeed. [And, yes, sorry… I apologize again to your old math teacher: he may not quite agree with the shortcut I am taking here, but he’ll justify the logicĀ behind.] So… Remembering thatĀ Ī»1Ā =Ā 2L, Ī»2Ā = L, Ī»3Ā =Ā (2/3)Ā·L, etcetera, we can then write:

E1Ā = (1/2)/L, E2Ā = (2/2)/L, E3Ā =Ā (3/2)/L, E4Ā =Ā (4/2)/L, E5Ā =Ā (5/2)/L,…, EnĀ =Ā (n/2)/L,…

That’s a reallyĀ nice result, because… Well… In quantum theory, we have this so-calledĀ equipartition theorem, which says that the permitted energy levels of a harmonic oscillator are equally spaced, with the interval between them equal to h or ħ (if you use the angular frequency to describe a wave (so that’s ω = 2π·f), then Planck’s constant (h) becomes ħ = h/2Ļ€). So here we’ve got equipartition too, with the interval between the various energy levels equal to (1/2)/L.

You’ll say: So what? Frankly, if this doesn’t amaze you, stop reading—but if this doesn’t amaze you, you actually stopped reading a long time ago. šŸ™‚ Look at what we’ve got here. WeĀ didn’t specify anything about that string, so we didn’t care about itsĀ materials or diameter or tension or how it was made (a wound guitar string is a terribly complicated thing!) or about whatever. Still, we know its fundamental (or normal) modes, and their frequency or nodes or energy or whatever depend on the length of the stringĀ only, with the ‘fundamental’ unit of energy being equal to the reciprocal length. Full stop. So all is just a matter of size and proportions. In other words, it’s all about structure. Absolute measurements don’t matter.

You may say: Bull****.Ā What’s the conclusion? You still didn’t tell me anything about how the total energy of the wave is supposed to be distributed over its normal modes!Ā 

That’s true. I didn’t. Why? Well… I am not sure, really. I presented a lot of stuff here, but I did notĀ present a clear and unambiguous answer as to how the total energy of a string is distributed over its modes. Not for actual strings, nor for idealĀ strings. Let me be honest: I don’t know. I really don’t. Having said that, my guts instinct that most of the energy – of, let’s say, a C4 note – should be in the primary mode (i.e. in the fundamental frequency) mustĀ be right: otherwise we would not call it a C4 note. So let’s try to make some assumptions. However, before doing so, let’s first briefly touch base with reality.

For actualĀ strings (orĀ actualĀ musical sounds), I suspect the analysisĀ can be quite complicated, as evidenced by the following illustration, which I took from one of the many interesting sitesĀ on this topic. Let me quote the author: “A flute is essentially a tube that is open at both ends. Air is blown across one end and sound comes out the other. The harmonics are all whole number multiples of the fundamental frequency (436Ā Hz, a slightly flat A4 — a bit lower in frequency than is normally acceptable). Note how the second harmonic is nearly as intense as the fundamental. [My = blog writer’s šŸ™‚ italics] This strong second harmonic is part of what makes a flute sound like a flute.”

Hmmm… What I see in the graph is a first harmonic that is actually moreĀ intense than its fundamental, so what’s that all about? So can we actually associate a specific frequency to that tone? Not sure. :-/ So we’re in trouble already.

flute

If reality doesn’t match our thinking, what about ideality? Hmmm… What to say?Ā As for idealĀ strings – or ideal flutes šŸ™‚Ā ā€“ I’d venture to say that the most obvious distribution of energy over the various modes (or harmonics, when we’re talking sound) would is theĀ Boltzmann distribution.

Huh?Ā Yes. Have a look at one of my posts on statistical mechanics. It’s a weird thing: the distribution of molecular speeds in a gas, or the density of the air in the atmosphere, or whatever involving many particles and/orĀ a great degree of complexity (so many, or such a degree of complexity, that only some kind of statistical approach to the problem works—all that involves Boltzmann’s Law, which basically says the distribution function will be a function of the energyĀ levels involved:Ā f =Ā e–energy. So… Well… Yes. It’s the logarithmic scale again. It seems to govern the Universe. šŸ™‚

Huh?Ā Yes. That’s why IĀ think: the distribution of the total energy of the oscillation should be some Boltzmann function, so it should depend on the energy of the modes: most of the energy will be in the lower modes, and most of the most in the fundamental. […]Ā Hmmm… It again begs the question: how muchĀ exactly?

Well… The BoltzmannĀ distribution stronglyĀ resemblesĀ the ‘harmonic’ distribution shown above (1, 1/2, 1/3, 1/4 etc), but it’s not quite the same. The graph below shows how they are similar and dissimilar in shape. You can experiment yourself with coefficients and all that, but your conclusion will be the same. As they say in Asia: they are “same-same but different.” šŸ™‚ […]Ā It’s like the ‘good’ and ‘equal’ temperament used when tuning musical instruments: the ‘good’ temperament – which isĀ based on harmonic ratios – is good, but not good enough. Only the ‘equal’ temperament obeys the logarithmic scale and, therefore, is perfect. So, as I mentioned already, while my assumption isn’t quite right (the distribution is notĀ harmonic, in the PythagoreanĀ sense), the intuition behind is OK. So it’s just like Pythagoras’ number theory of the Universe. Having said that, I’ll leave it to you to draw the correct the conclusions from it. šŸ™‚

graph

Music and Physics

Pre-scriptum (dated 26 June 2020): These posts on elementary math and physics have not suffered much the attack by the dark force—which is good because I still like them. While my views on the true nature of light, matter and the force or forces that act on them have evolved significantly as part of my explorations of a more realist (classical) explanation of quantum mechanics, I think most (if not all) of the analysis in this post remains valid and fun to read. In fact, I find the simplest stuff is often the best. šŸ™‚

Original post:

My first working title for this post was Music andĀ Modes. Yes. Modes. Not moods. The relation between music and moods is an interesting research topic as well but so it’s not what I am going to write about. šŸ™‚

It started with me thinking I should write something on modes indeed, because the concept of aĀ modeĀ of a wave, or any oscillator really, is quite central to physics, both in classical physics as well as in quantum physics (quantum-mechanical systems are analyzed as oscillators too!). But I wondered how to approach it, as it’s a rather boring topic if you look at the math only. But thenĀ I was flying back from Europe, to Asia, where I live and, as I am also playing a bit of guitar, I suddenly wanted to know why we like music. And then I thought that’s a question you may have asked yourself at some point of time too! And so then I thought I should write about modes as part of a more interesting story: a story aboutĀ music—or, to be precise, a story about the physics behind music. So… Let’s go for it.

Philosophy versus physics

There is, of course, a very simple answer to the question of why we like music: we like music because it is music. If it would notĀ be music, we would notĀ like it. That’s a rather philosophical answer, and it probably satisfies most people. However, for someone studying physics, that answer can surely not be sufficient.Ā What’s the physics behind? I reviewed Feynman’sĀ LectureĀ on sound waves in the plane, combined it with some other stuff I googledĀ when I arrived, and then I wrote this post, which gives you a much less philosophical answer. šŸ™‚

The observation at the center of the discussion is deceptively simple: why is it that similar strings (i.e. strings made of the same material, with the same thickness, etc), under the same tension but differing in length, sound ‘pleasant’ when sounded together if – and only if  – the ratio of the length of the strings is like 1:2, 2:3, 3:4, 3:5, 4:5, etc (i.e. like whatever other ratio of two small integers)?

You probably wonder: is that the question, really? It is. The question is deceptively simple indeed because, as you will see in a moment, the answer is quite complicated. SoĀ complicated, in fact, that the Pythagoreans didn’t have any answer. Nor did anyone else for that matter—until the 18th century or so, when musicians, physicists and mathematicians alike started to realize that a string (of a guitar, or a piano, or whatever instrument Pythagoras was thinking of at the time),Ā or a column of air (in a pipe organ or a trumpet, for example), or whatever other thing that actually creates the musical tone, actuallyĀ oscillates at numerous frequencies simultaneously.

The Pythagoreans did not suspect that a string, in itself, is a rather complicated thing – something which physicists refer to as a harmonic oscillator – and that its sound, therefore, is actually produced by many frequencies, instead of only one. The concept of a pure note, i.e. a tone that is free of harmonics (i.e. free of all other frequencies, except for the fundamentalĀ frequency) also didn’t exist at the time. And if it did, they would not have been able to produce a pure tone anyway: producing pure tones – or notes, as I’ll call them, somewhat inaccurately (I should say: a pureĀ pitch) – is remarkably complicated, and they do not exist in Nature. If the Pythagoreans would have been able to produce pure tones, they would have observed that pure tones doĀ notĀ give any sensation of consonance or dissonance if their relative frequencies respect those simple ratios. Indeed, repeated experiments, in which such pure tones are being produced, have shown that human beings can’t really say whether it’s a musical sound or not: it’s just sound, and it’s neither pleasant (or consonant, we should say)Ā or unpleasant (i.e. dissonant).

The Pythagorean observation isĀ valid, however, for actual (i.e. non-pure)Ā musical tones. In short, we need to distinguish betweenĀ tones and notes (i.e. pure tones): theyĀ are two very different things, and the gist of the whole argument is that musical tones coming out of one (or more) string(s) under tension are full of harmonics and, as I’ll explain in a minute, that’s what explains the observed relation between the lengths of those strings and the phenomenon of consonanceĀ (i.e. sounding ‘pleasant’) or dissonanceĀ (i.e.Ā sounding ‘unpleasant’).

Of course, it’s easy to say what I say above: we’re 2015 now, and so we have the benefit of hindsight. Back then – Ā so that’s more than 2,500 years ago! – the simple but remarkableĀ fact that the lengths of similar strings should respect some simple ratio if they are to sound ‘nice’ together, triggered a fascination with number theory (in fact, the Pythagoreans actually established the foundations of what is now known as number theory). Indeed, Pythagoras felt that similar relationships should also hold for other natural phenomena! To mention just one example, the Pythagoreans also believed that the orbits of the planets would also respect such simple numerical relationships, which is why they talked of the ‘music of the spheres’ (Musica Universalis).

We now know that the Pythagoreans wereĀ wrong. TheĀ proportions in the movements of the planets around the Sun do not respect simple ratios and, with the benefit of hindsight once again, it is regrettable that it took many courageous and brilliant people, such as Galileo Galilei and Copernicus, to convince the Church of that fact. 😦 Also, while Pythagoras’ observations in regard to the sounds coming out of whatever strings he was looking at were correct, his conclusions were wrong: the observation does notĀ imply that the frequencies of musical notesĀ should all be in some simple ratio one to another.

Let me repeat what I wrote above: the frequencies of musical notesĀ are notĀ in some simple relationship one to another. The frequency scale for all musical tones is logarithmic and, while that implies that we can, effectively, do some tricks with ratios based on the properties of the logarithmic scale (as I’ll explain in a moment), the so-called ‘Pythagorean’ tuning system, which is based on simple ratios, was plain wrong, even if it – or some variant of it (instead of the 3:2 ratio, musicians used the 5:4 ratio from about 1510 onwards) – was generally used until the 18th century!Ā In short, Pythagoras was wrong indeed—in this regard at least: we can’t do much with those simple ratios.

Having said that, Pythagoras’ basic intuition was right, and that intuition is still very much what drives physics today: it’s the idea that Nature can be described, or explained (whatever that means), by quantitative relationships only. Let’s have a look at how it actually works for music.

Tones, noise and notes

Let’s first define and distinguish tones and notes.Ā A musical tone is the opposite of noise, and the difference between the two is that musical tones areĀ periodicĀ waveforms, so they have aĀ periodĀ T, as illustrated below. In contrast, noise is a non-periodic waveform. It’s as simple as that.

noise versus music

Now, from previous posts, you know we can write any period function as the sum of a potentially infinite number of simple harmonic functions, and that this sum is referred to as the Fourier series. I am just noting it here, so don’t worry about it as for now. I’ll come back to it later.

You also know we have seven musical notes: Do-Re-Mi-Fa-Sol-La-Si or, more common in the English-speaking world, A-B-C-D-E-F-G. And then it starts again with A (or Do). So we have two notes, separated by an interval which is referred to as an octaveĀ (from the GreekĀ octo, i.e. eight), with six notes in-between, so that’s eight notes in total. However, you also know that there are notes in-between, except between E and F and between B and C. They are referred to as semitones or half-steps. I prefer the term ‘half-step’ over ‘semitone’, because we’re talking notes really, not tones.

We have, for example, F–sharpĀ (denoted by F#), which we can also call G-flat (denoted by Gb). It’s the same thing: a sharp # raises a note by a semitone (aka half-step), and a flat b lowers it by the same amount, so F# is Gb. That’s what shown below: in an octave, we have eight notes but twelve half-steps.Ā 

Frequency_vs_name

Let’s now look at the frequencies. The frequencyĀ scale above (expressed in oscillations per second, so that’s the hertz unit) is a logarithmic scale: frequenciesĀ doubleĀ as we go from one octave to another: the frequency of the C4 note above (the so-called middle C)Ā is 261.626 Hz, while the frequency of the next C note (C5) is double that: 523.251 Hz. [Just in case you’d want to know: the 4 and 5 number refer to its position on a standard 88-key piano keyboard: C4 is the fourth C key on the piano.]

Now, if we equate the interval between C4 and C5 with 1 (so the octave is our musical ‘unit’), then the interval between the twelve half-steps is, obviously, 1/12. Why? Because we have 12 halve-steps in our musical unit. You can also easily verify that, because of the way logarithms work, theĀ ratio of the frequencies of two notes that are separated by one half-step (between D# and E, for example) will be equal to 21/12. Likewise, the ratio of the frequencies of two notes that are separated by nĀ half-steps is equal to 2n/12. [In case you’d doubt, just do an example. For instance, if we’d denote the frequency of C4 asĀ f0, and the frequency of C# as f1Ā and so on (so the frequency of D is f2, the frequency of C5 is f12, and everything else is in-between), then we can write the f2/f0Ā ratio asĀ f2/f0Ā = (Ā f2/f1)(f1/f0) = Ā 21/12Ā·21/12Ā = 22/12Ā = 21/6. I must assume you’re smart enough to generalize this result yourself, and thatĀ f12/f0Ā is, obviously, equal toĀ 212/12Ā =21Ā = 2, which is what it should be!]

Now, because the frequencies of the various C notes are expressed as a number involving some decimal fraction (likeĀ 523.251 Hz, and the 0.251 is actually an approximation only), and because they are, therefore, a bit hard to read and/or work with, I’ll illustrate the next idea – i.e. the concept of harmonics – with the A instead of the C. šŸ™‚

Harmonics

The lowest A on a piano is denoted by A0, and its frequency is 27.5 Hz. Lower A notes exist (we have one at 13.75 Hz, for instance) but we don’t use them, because they are near (or actually beyond) the limit of the lowest frequencies we can hear. So let’s stick to our grand piano and start with that 27.5 Hz frequency. The next A note is A1, and its frequency is 55 Hz. We then have A2, which is like the A on my (or your) guitar: its frequency is equal to 2Ɨ55 = 110 Hz. The next is A3, for which we double the frequency once again: we’re at 220 Hz now. The next one is the A in the illustration of the C scale above: A4, with a frequency of 440 Hz.

[Let me, just for the record, note that the A4Ā note is the standard tuning pitchĀ in Western music. Why? Well… There’s no good reason really, except convention. Indeed,Ā we can derive the frequency of any other note from that A4Ā note using our formula for the ratio of frequencies but, because of the properties of a logarithmic function, we could do the same using whatever other note really. It’s an important point: there’s no such thing as an absolute reference point in music: once we defineĀ our musical ‘unit’ (so that’s the so-called octave in Western music), and how many steps we want to have in-between (so that’s 12 steps—again, in Western music, that is), we get all the rest. That’s just how logarithms work. So music is all about structure, i.e. mathematical relationships. Again, Pythagoras’ conclusions were wrong, but his intuition was right.]

Now, the notes we are talking about here are all so-called pure tones. In fact, when I say that the A on our guitar is referred to as A2Ā and that it has a frequency of 110 Hz, then I am actually making a huge simplification. Worse, I am lying when I say that: when you play a string on a guitar, or when you strike a key on a piano, all kinds of other frequencies – so-called harmonics – will resonate as well, and that’s what gives the quality to theĀ sound: it’s what makes it sound beautiful. So the fundamental frequency (aka asĀ first harmonic) is 110 Hz alright but we’ll also have second, third, fourth, etc harmonics with frequency 220 Hz, 330 Hz, 440 Hz, etcetera. In music, the basic or fundamental frequency is referred to as the pitch of the tone and, as you can see, I often use the term ‘note’ (or pureĀ tone)Ā as a synonym for pitch—which is more or less OK, but not quite correct actually. [However, don’t worry about it: my sloppiness here does not affect the argument.]

What’s the physics behind? Look at the illustration below (I borrowed it from theĀ Physics ClassroomĀ site). The thick black line is the string, and the wavelength of its fundamental frequency (i.e. the first harmonic) isĀ twiceĀ its length, so we write Ī»1Ā = 2Ā·L or, the other way around, L = (1/2)Ā·Ī»1. Now that’s the so-called first modeĀ of the string. [One often sees the term fundamentalĀ orĀ natural or normalĀ mode, but the adjective is not necessary really. In fact, I find it confusing, although I sometimes find myself using it too.]

string

We also have a second, third, etc mode, depicted below, and these modes correspond to the second, third, etc harmonic respectively.

modes

For the second, third, etc mode, the relationship between the wavelength and the length of the string is, obviously, the following: L = (2/2)·λ2 = λ2, L = L = (3/2)·λ3, etc. More in general, for the nth mode, L will be equal to L = (n/2)·λn, with n = 1, 2, etcetera. In fact, because L is supposed to be some fixed length, we should write it the other way around: λn = (2/n)·L.

What does it imply for the frequencies? We know that theĀ speedĀ of the wave – let’s denote it by c – as it travels up and down the string, is a property of the string,Ā and it’s a propertyĀ of the string only. In other words, it doesĀ notĀ depend on the frequency. Now, the wave velocity is equal to the frequency times the wavelength,Ā always, so we have c = fĀ·Ī». To take the example of the (classical) guitar string: its length is 650 mm, i.e. 0.65 m. Hence, the identities Ī»1Ā = (2/1)Ā·L,Ā Ī»2Ā = (2/2)Ā·L,Ā Ī»3Ā = (2/3)Ā·L etcĀ become Ī»1Ā = (2/1)Ā·0.65 = 1.3 m, Ī»2Ā = (2/2)Ā·0.65 = 0.65 m, Ī»3Ā = (2/3)Ā·0.65 = 0.433.. m and so on. Now, combining these wavelengths with the above-mentioned frequencies, we get the wave velocity c = (110 Hz)Ā·(1.3 m) = (220 Hz)Ā·(0.65 m) = (330 Hz)Ā·(0.433.. m) = 143 m/s.

Let me now get back to Pythagoras’ string. You should note that the frequencies of the harmonics produced by a simple guitar string are related to each other by simple whole number ratios. Indeed, the frequencies of the first and second harmonics are in a simple 2 to 1 ratio (2:1). The second and third harmonics have a 3:2 frequency ratio. The third and fourth harmonics a 4:3 ratio. The fifth and fourth harmonic 5:4, and so on and so on. They have to be. Why?Ā Because the harmonics are simple multiples of the basic frequency. NowĀ thatĀ is what’s really behind Pythagoras’ observation: when he was sounding similar strings with the same tension but different lengths, he was making sounds with the same harmonics. Nothing more, nothing less.Ā 

Let me be quite explicit here, because the point that I am trying to make here is somewhat subtle. Pythagoras’ string is Pythagoras’ string: he talked similar strings. So we’re not talking some actual guitar or a piano or whatever other string instrument. The strings on (modern) string instruments are not similar, and they do notĀ have the same tension.Ā For example, the six strings of a guitar strings doĀ notĀ differ in length (they’re all 650 mm) but they’re differentĀ in tension. The six strings on a classical guitar also have a different diameter, and the first three strings are plain strings, as opposed to the bottom strings, which are wound. So the strings are not similar but very different indeed. To illustrate the point, I copied the values below for just one of the many commercially available guitar string sets.Ā Ā tensionIt’s the same for piano strings. While they are somewhat more simple (they’re all made of piano wire, which is very high quality steel wire basically), they alsoĀ differ—not only in length but in diameter as well, typically ranging fromĀ 0.85Ā mm for the highest treble strings to 8.5Ā mm (so that’s ten times 0.85 mm) for the lowest bass notes.

In short, Pythagoras wasĀ notĀ playing the guitar or the piano (or whatever other more sophisticated string instrument that the Greeks surely must have had too) when he was thinking of these harmonic relationships. The physical explanation behind his famous observation is, therefore, quite simple: musical tones that have the same harmonics sound pleasant,Ā or consonant, we should say—from the LatinĀ con-sonare, which, literally, means ‘to sound together’ (from sonare = to sound and con = with). And otherwise… Well… Then they doĀ notĀ sound pleasant: they are dissonant.

To drive the point home, let me emphasize that, when we’re plucking a string, we produce a sound consisting of many frequencies, all in one go. One can see it in practice: if you strike a lower A string on a piano – let’s say the 110 Hz A2Ā string – then its second harmonic (220 Hz) will make the A3Ā string vibrate too, because it’s got the same frequency! And then its fourthĀ harmonic will make the A4Ā string vibrate too, because they’re both at 440 Hz.Ā Of course, the strength of these other vibrations (or their amplitudeĀ we should say)Ā will depend on the strength of the other harmonics and we should, of course, expect that theĀ fundamentalĀ frequency (i.e. the first harmonic) will absorb most of the energy. So we pluck one string, and so we’ve got one sound, oneĀ tone only, but numerousĀ notesĀ at the same time!

In this regard,Ā you should also note thatĀ theĀ third harmonic of our 110 Hz A2Ā string corresponds to the fundamental frequency of the E4 tone: both are 330 Hz! And, of course, the harmonics of E, such as its second harmonic (2Ā·330 Hz = 660 Hz) correspond to higher harmonics of A too! To be specific, the second harmonic of our E string is equal to the sixth harmonic of our A2Ā string. If your guitar is any good,Ā and if your strings are of reasonable quality too, you’ll actually see it: the (lower) E and A strings co-vibrate if you play the A major chord, but by striking the upper four strings only. So we’ve got energy – motion really – being transferred from the four strings you do strike to the two strings you doĀ not strike! You’ll say: so what? Well… If you’ve got any better proof of the actuality (or reality)Ā of various frequencies being present at the same time, please tell me! šŸ™‚

So that’s why A and E sound veryĀ well together (A, E and C#, played together, make up the so-called A major chord): our ear likes matching harmonics. And so thatĀ why we like musical tones—or why we define those tones as being musical! šŸ™‚ Let me summarize it once more: musical tones are composite sound waves, consisting of a fundamental frequency and so-called harmonics (so we’ve got many notesĀ or pure tones altogether in one musicalĀ tone). Now, when other musical tones have harmonics that are shared, and we sound those notes too, we get the sensation of harmony, i.e. the combination soundsĀ consonant.

Now, i’s not difficult to see that we will always have such shared harmonics if we haveĀ similar strings, with the same tension but different lengths, being sounded together. In short, what Pythagoras observed has nothing much to do withĀ notes, but withĀ tones.Ā Let’s go a bit further in the analysis now by introducing some more math. And, yes, I am very sorry: it’s the dreaded Fourier analysis indeed! šŸ™‚

Fourier analysis

You know that we can decompose any periodic function into a sum of a (potentially infinite) series of simple sinusoidal functions, as illustrated below. I took the illustration from Wikipedia: the red function s6(x) is the sum of six sine functions of different amplitudes and (harmonically related) frequencies. The so-called Fourier transformĀ S(f) (in blue) relates the six frequencies with the respective amplitudes.

Fourier_series_and_transform

In light of the discussion above, it is easy to see what this means for the sound coming from a plucked string. Using the angular frequency notation (so we write everything using ω instead of f), we know that the normal or natural modes of oscillation have frequencies ω = 2Ļ€/T = 2Ļ€fĀ Ā (so that’s the fundamental frequency or first harmonic), 2ω (second harmonic), 3ω (third harmonic), and so on and so on.

Now, there’s no reason to assume that all of the sinusoidal functions that make up our tone should have the same phase: some phase shift Φ may be there and, hence, we should write our sinusoidal function Ā not as cos(ωt), but as cos(ωt + Φ) in order to ensure our analysis is general enough.Ā [Why not a sine function? It doesn’t matter: the cosine and sine function are the same, except for another phase shift of 90° = π/2.] Now, from our geometry classes, we know that we can re-write cos(ωt + Φ) as

cos(ωt + Φ) = [cos(Φ)cos(ωt) – sin(Φ)sin(ωt)]

We have a lot of these functions of course – one for each harmonic, in fact – and, hence, we should use subscripts, which is what we do in the formula below, which says thatĀ any function f(t) that is periodic with the period T can be written mathematically as:

Fourier series

You may wonder: what’s that period T? It’s the period of the fundamental mode, i.e. the first harmonic. Indeed, the period of the second, third, etc harmonic will only be one half, one third etcetera of the period of the first harmonic. Indeed, T2Ā = (2Ļ€)/(2ω) = (1/2)Ā·(2Ļ€)/ω = (1/2)Ā·T1, andĀ T3Ā = (2Ļ€)/(3ω) = (1/3)Ā·(2Ļ€)/ω = (1/3)Ā·T1, and so on. However, it’s easy to see that these functions alsoĀ repeat themselves after two, three, etc periods respectively. So all is alright, and the general idea behind the Fourier analysis is further illustrated below. [Note that both the formula as well as the illustration below (which I took from Feynman’s Lectures)Ā add a ‘zero-frequency term’ a0Ā to the series. That zero-frequency term will usually be zero for a musical tone, because the ‘zero’ level of our tone will be zero indeed. Also note that the anĀ and bnĀ coefficients are, of course, equal to anĀ = cos ΦnĀ and bnĀ = –sinΦn, so you can relate the illustration and the formula easily.]

Fourier 2You’ll say: What the heck!Ā Why do we need the mathematical gymnastics here? It’s just to understand that other characteristic of a musical tone: its qualityĀ (as opposed to its pitch). A so-called richĀ tone will have strong harmonics, while aĀ pureĀ tone will only have the first harmonic. All other characteristics – the difference between a tone produced by a violin as opposed to a piano – are then related to the ‘mix’ of all those harmonics.

So we have it all now, except for loudness which is, of course, related to the magnitude of the air pressure changes as our waveform moves through the air: pitch, loudness and quality. that’s what makes a musical tone. šŸ™‚

Dissonance

As mentioned above, if the sounds are not consonant, they’re dissonant. But what is dissonance really? What’s going on? The answer is the following: whenĀ two frequencies are near to a simple fraction, but not exact, we get so-called beats, which our ear does notĀ like.

Huh?Ā Relax.Ā The illustration below, which I copied from the Wikipedia article on piano tuning, illustrates the phenomenon.Ā The blue wave is the sum of the red and the green wave, which are originally identical. But then the frequency of the green wave is increased, and so the two waves are no longer in phase, and the interference results in a beating pattern. Of course, our musical tone involves different frequencies and, hence, different periodsĀ T1,T2,Ā T3Ā etcetera, but you get the idea: the higher harmonics alsoĀ oscillate with period T1, and if the frequencies are notĀ in some exact ratio, then we’ll have a similar problem: beats, and our ear will not like the sound.

220px-WaveInterference

Of course, you’ll wonder: why don’t we like beats in tones? We can ask that, can’t we? It’s like asking why we like music, isn’t it? […] Well… It is and it isn’t. It’s like asking why our ear (or our brain) likes harmonics. We don’t know. That’s how we are wired. The ‘physical’ explanation of what is musical and what isn’t only goes so far, I guess. 😦

Pythagoras versus Bach

From all of what I wrote above, it is obvious that the frequencies of theĀ harmonics of a musical tone are, indeed, related by simple ratios of small integers: the frequencies of the first and second harmonics are in a simple 2 to 1 ratio (2:1); the second and third harmonics have a 3:2 frequency ratio; the third and fourth harmonics a 4:3 ratio; the fifth and fourth harmonic 5:4, etcetera. That’s it. Nothing more, nothing less.

In other words, Pythagoras was observing musical tones: he could notĀ observe the pure tonesĀ behind, i.e. the actualĀ notes.Ā However, aesthetics led Pythagoras, and all musicians after him – until the mid-18th century – to also think that the ratio of the frequencies of the notes within an octaveĀ should also be simple ratios. From what I explained above, it’s obvious that it should notĀ work that way: the ratio of the frequencies of two notes separated by n half-steps is 2n/12, and, for most values of n, 2n/12Ā is not some simple ratio. [Why? Just take your pocket calculator and calculate the value of 21/12: it’s 20.08333…Ā = 1.0594630943… and so on… It’s an irrational number: there are no repeating decimals. Now,Ā 2n/12Ā is equal to 21/12Ā·21/12Ā·…Ā·21/12Ā (n times). Why would you expect that product to be equal to some simple ratio?]

So – I said it already – Pythagoras was wrong—not only in this but also in other regards, such as when he espoused his views on the solar system, for example. Again, I am sorry to have to say that, but it is what is: the Pythagoreans did seem to prefer mathematical ideas over physical experiment.Ā šŸ™‚Ā Having said that, musicians obviously didn’t know about any alternative to Pythagoras, and they had surely never heard about logarithmic scales at the time. So… Well… They did use the so-called Pythagorean tuning system.Ā To be precise, they tuned their instruments by equating the frequency ratio between the first and the fifth tone in the C scaleĀ (i.e. the C and G, as they did notĀ include the C#, D# and F#Ā semitones when counting) with the ratioĀ 3/2, and then they used other so-called harmonic ratios for the notes in-between.

Now, the 3/2 ratio is actuallyĀ almostĀ correct, because the actual frequency ratio isĀ 27/12Ā (we have seven tones, including the semitones—not five!), and so that’s 1.4983, approximately. Now, that’s pretty close to 3/2 = 1.5, I’d say. šŸ™‚ Using that approximation (which, I admit, is fairly accurate indeed), the tuning of the other strings would then also be done assuming certain ratios should be respected, like the ones below.

Capture

So it was all quiteĀ good.Ā Having said that, good musicians, and some great mathematicians, felt something was wrong—if only because there were several so-called just intonationĀ systems around (for an overview, check out the Wikipedia article on just intonation). More importantly, they felt it was quite difficult toĀ transposeĀ music using the Pythagorean tuning system. Transposing music amounts to changing the so-calledĀ keyĀ of a musical piece: what one does, basically, is moving the whole piece up or down in pitch by some constant interval that is not equal to anĀ octave. Today, transposing music is a piece of cake—Western music at least. But that’s only because all Western music is played on instruments that are tuned usingĀ that logarithmic scale (technically, it’s referred to as the 12-tone equal temperament (12-TET) system). When you’d use one of the Pythagorean systems for tuning, a transposed piece does notĀ sound quite right.Ā 

The first mathematician who really seemed to know what was wrong (and, hence, who also knew what to do) was Simon Stevin, who wrote a manuscript based on the ’12thĀ root of 2 principle’ around AD 1600. It shouldn’t surprise us: the thinking of this mathematician from Bruges would inspire John Napier’s work on logarithms. Unfortunately, while that manuscript describes the basic principles behind the 12-TET system, it didn’t get published (Stevin had to run away from Bruges, to Holland, because he was protestant and the Spanish rulers at the time didn’t like that). Hence, musicians, while not quite understanding the mathĀ (or the physics, I should say) behind their own music, kept trying other tuning systems, as they felt it made their music sound better indeed.

One of these ‘other systems’ is the so-calledĀ ‘good’Ā temperament, which you surely heard about, as it’sĀ referred to in Bach’s famous composition, Das Wohltemperierte Klavier, which he finalized in the first half of the 18th century. What is that ‘good’ temperament really? Well… It is what it is: it’s one of those tuning systems which made musicians feel better about their music for a number of reasons, all of which are well described in the Wikipedia article on it. But the main reason is that the tuning system that Bach recommended was a great deal better when it came to playing the same piece in another key. However, it still wasn’t quite right, as it wasn’t theĀ equal temperamentĀ system (i.e. the 12-TET system) that’s in place now (in the West at least—the Indian music scale, for instance, is still based on simple ratios).

Why do I mention this piece of Bach? The reason is simple: you probably heard of it because it’s one of the main reference points in a rather famous book: Gƶdel, Escher and Bach—an Eternal Golden Braid. If not, then just forget about it. I am mentioning it because one of my brothers loves it. It’s on artificial intelligence. I haven’t read it, but I must assume Bach’s master piece is analyzed there because of its structure, not because of the tuning system that one’s supposed to use when playing it. So… Well… I’d say: don’t make that composition any more mystic than it already is. šŸ™‚ The ‘magic’ behind it is related to what I said about A4 being the ‘reference point’ in music: since we’re using a universal logarithmic scale now, there’s no such thing as an absolute reference point any more: once we defineĀ our musical ‘unit’ (so that’s the so-called octave in Western music), and also define how many steps we want to have in-between (so that’s 12—in Western music, that is), we get all the rest. That’s just how logarithms work.

So, in short, music is all about structure, i.e. it’s all aboutĀ mathematical relations, and about mathematical relations only. Again, Pythagoras’ conclusions were wrong, but his intuition was right. And, of course, it’s his intuition that gave birth to science: the simple ‘models’ he made – of how notes are supposed to be related to each other, or about our solar system – were, obviously, just the start of it all. And what a great start it was! Looking back once again, it’s rather sad conservative forces (such as the Church) often got in the way of progress. In fact, I suddenly wonder: if scientists would not have been bothered by those conservative forces, could mankind have sent people around the time that Charles V was born, i.e. around A.D. 1500 already? šŸ™‚

Post scriptum:Ā My example of theĀ the (lower) E and A guitar strings co-vibrating when playing the A major chordĀ striking the upper four strings only, is somewhat tricky. The (lower) E and A strings are associated with lowerĀ pitches, and we said overtones (i.e. the second, third, fourth, etc harmonics) are multiplesĀ of the fundamental frequency.Ā So why is that the lowerĀ strings co-vibrate? The answer is easy: they oscillate at the higher frequencies only. If you have a guitar: just try it. The two strings you do not pluck do vibrate—and very visibly so, but the low fundamental frequencies that come out of them when you’d strike them, are not audible. In short, they resonate at the higher frequencies only. šŸ™‚

The example that Feynman gives is much more straightforward: his example mentions the lower C (or A, B, etc) notes on a piano causing vibrations in the higher C strings (or the higher A, B, etc string respectively). For example, striking the C2 key (and, hence, the C2 string inside the piano) will make the (higher) C3 string vibrate too. But few of us have a grand piano at home, I guess. That’s why I prefer my guitar example. šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Maxwell-Boltzmann, Bose-Einstein and Fermi-Dirac statistics

Pre-scriptum added much later: We have advanced much in our understanding since we wrote this post. If you are reading it because you want to understand more about the boson-fermion distinction, then you shouldn’t be here.Ā The general distinction between bosons and fermions is a useless theoretical generalization which actually preventsĀ you from understanding what is really going on. I am keeping this post online for documentation purposes only. It is interesting from a math point of view but you are not here to learn math, are you?

Jean Louis Van Belle, 20 May 2020

Original post:

I’ve discussed statistics, in the context of quantum mechanics, a couple of times already (see, for example, my post on amplitudes and statistics). However, I never took the time to properly explain those distribution functions which are referred to as the Maxwell-Boltzmann, Bose-Einstein and Fermi-Dirac distribution functions respectively. Let me try to do that now—without, hopefully, getting lost in too much math! It should be a nice piece, as it connects quantum mechanics with statistical mechanics, i.e. two topics I had nicely separated so far. šŸ™‚

You know the Boltzmann Law now, which says that the probabilities of different conditions of energy are given by eāˆ’energy/kTĀ = 1/eenergy/kT. Different ‘conditions of energy’ can be anything: density, molecular speeds, momenta, whatever. The point is: we have some probability density function f, and it’s a function of the energy E, so we write:

f(E) = CĀ·eāˆ’energy/kTĀ = C/eenergy/kT

C is just a normalization constant (all probabilities have to add up to one, so the integral of this function over its domain must be one), and k and T are also usual suspects: T is the (absolute) temperature, and k is the Boltzmann constant, which relates the temperate to the kinetic energy of the particles involved.Ā We also know the shape of this function. For example, when we applied it to the density of the atmosphere at various heights (which are related to the potential energy, as P.E. = mĀ·gĀ·h), assuming constant temperature, we got the following graph.Ā The shape of this graph is that of an exponential decay function (we’ll encounter it again, so just take a mental note of it).

graph

A more interesting application is the quantum-mechanical approach to the theory of gases, which I introduced in my previous post. To explain the behavior of gases under various conditions, we assumed that gas molecules are like oscillators but that they can only take on discrete levels of energy. [That’s what quantum theory is about!]Ā We denoted the various energy levels, i.e. the energies of the various molecular states, by E0, E1, E2,…,Ā Ei,…, and if Boltzmann’s Law applies, then the probability of finding a molecule in the particular state EiĀ is proportional toĀ eāˆ’EiĀ /kT.Ā We can then calculate the relativeĀ probabilities, i.e. the probability of being in stateĀ Ei, relative to the probability of being in state E0, is:

Pi/P0Ā = eāˆ’EiĀ /kT/eāˆ’E0Ā /kTĀ = eāˆ’(Ei–E0)/kTĀ = 1/e(Ei–E0)/kT

Now, PiĀ obviously equals ni/N, so it is the ratio of the number of molecules in state EiĀ (ni)Ā and the total number of molecules (N). Likewise, P0Ā = n0/N and, therefore, we can write:

ni/n0Ā =Ā eāˆ’(Eiāˆ’E0)/kTĀ = 1/e(Ei–E0)/kT

This formulation is just another Boltzmann Law, but it’s nice in that it introduces the idea of a ground state, i.e. the state with the lowest energy level. We may or may not want to equateĀ E0Ā with zero. It doesn’t matter really: we can always shift all energies by some arbitrary constant because we get to choose the reference point for the potential energy.

So that’s the so-called Maxwell-Boltzmann distribution.Ā Now, in my post on amplitudes and statistics, I had jotted down the formulas for the other distributions, i.e. the distributions when we’re not talking classical particles butĀ fermions and/or bosons.Ā As you know, fermions are particles governed by the Fermi exclusion principle: indistinguishable particles cannot be together in the same state. For bosons, it’s the other way around: having one in some quantum state actually increases the chance of finding another one there, and we can actually have an infinite number of them in the same state.

We also know that fermions and bosons are theĀ realĀ world: fermions are the matter-particles, bosons are the force-carriers, and our ‘Boltzmann particles’ are nothing but a classical approximation of the real world. Hence, even if we can’t see them in the actual world, the Fermi-Dirac and Bose-Einstein distributions are the real-world distributions. šŸ™‚ Let me jot down the equations once again:

Fermi-Dirac (for fermions): f(E)Ā = 1/[Ae(EĀ āˆ’ EF)/kTĀ + 1]

Bose-Einstein (for bosons):Ā  f(E)Ā = 1/[AeE/kTĀ āˆ’ 1]

We’ve got some other normalization constant here (A), which we shouldn’t be too worried about—for the time being, that is. Now, to see how these distributions are different from the Maxwell-Boltzmann distribution (which we should re-write asĀ f(E) = CĀ·eāˆ’E/kTĀ = 1/[AĀ·eE/kT] so as to make all formulas directly comparable), we should just make a graph. Please go online to find a graph tool (I found a new one recently—really easy to use), and just do it. You’ll see they are all like that exponential decay function. However, in order to make a proper comparison, we would actually need to calculate the normalization coefficients and, for the Fermi energy, we would also need the Fermi energy EFĀ (note that, for simplicity, we did equateĀ E0Ā with zero). Now, we could give it a try, but it’s muchĀ easier to googleĀ and find an example online.

TheĀ HyperPhysicsĀ website of Georgia State University gives us one: the example assumes 6 particles and 9 energy levels, and the table and graph below compare the Maxwell-Boltzmann and Bose-Einstein distributions for the model.

Graph Table

Now thatĀ is an interesting example, isn’t it? In this example (but all depends on its assumptions, of course), the Maxwell-Boltzmann and Bose-Einstein distributions are almost identical. Having said that, we can clearly see that the lower energy states are, indeed, more probable with Bose-Einstein statistics than with the Maxwell-Boltzmann statistics. While the difference is not dramatic at all in this example, the difference does become very dramatic, in reality,Ā with large numbers (i.e. high matter density) and, more importantly, at very low temperatures, at which bosons can condense into the lowest energy state. This phenomenon is referred to as Bose-Einstein condensation: it causes superfluidity and superconductivity, and it’s real indeed:Ā it has been observed with supercooled He-4, which is notĀ an everyday substance, but real nevertheless!

What about the Fermi-Dirac distribution for this example? The Fermi-Dirac distribution is given below: the lowest energy state is nowĀ less probable, the mid-range energies muchĀ more, and none of the six particles occupy any of the four highest energy levels. Again, while the difference is not dramatic in this example, it can become very dramatic, in reality,Ā with large numbers (read: high matter density) and very low temperatures: at absolute zero, all of the possible energy states up to the Fermi energy level will be occupied, and all the levels above the Fermi energy will be vacant.

graph 2 Table 2

What can we make out of all of this? First, you may wonder why we actually have more than one particle in one state above: doesn’t that contradict the Fermi exclusion principle? No. We need to distinguish micro- and macro-states. In fact, the example assumes we’re talking electrons here, and so we can have two particles in each energy state—with opposite spin, however. At the same time, it’s true we cannot have three, or more, in any state.Ā That results, in the example we’re looking at here, in five possible distributions only, as shown below.

Table 3

The diagram is an interesting one: if the particles were to be classical particles, or bosons,Ā then 26 combinations are possible, including the five Fermi-Dirac combinations, as shown above. Note the little numbers above the 26 possible combinations (e.g. 6, 20, 30,… 180): they are proportional to the likelihood of occurring under the Maxwell-Boltzmann assumption (so if we assume the particles are ‘classical’ particles).Ā Let me introduce you to the math behind the example by using the diagram below, which shows threeĀ possible distributions/combinations (I know the terminology is quite confusing—sorry for that!).

table 4

If we could distinguish the particles, then we’d have 2002 micro-states, which is the total of all those little numbers on top of the combinations that are shown (6+60+180+…). However, the assumption is that we cannot distinguish the particles. Therefore, the first combination in the diagram above, with five particles in the zero energy state and one particle in state 9, occurs 6 times into 2002 and, hence, it has a probability of 6/2002Ā ā‰ˆ 0.003 only. In contrast, the second combination is 10 times more likely, and the third one is 30 times more likely! In any case, the point is, in the classical situation (and in the Bose-Einstein hypothesis as well), we have 26 possible macro-states, as opposed to 5 only for fermions, and so that leads to a very different density function.Ā Capito?

No? Well, this blog is not a textbook on physics and, therefore, I should refer you to the mentioned site once again, which references a 1992 textbook on physics (Frank Blatt, Modern Physics, 1992) as the source of this example. However, I won’t do that: you’ll find the details in the Post ScriptumĀ to this post. šŸ™‚

Let’s first focus on the fundamental stuff, however.Ā The most burning question is: if the real world consists of fermions and bosons, why is that that we only see the Maxwell-Boltzmann distribution inĀ our actualĀ (non-real?)Ā world? šŸ™‚ The answer is that both the Fermi-Dirac and Bose-Einstein distribution approach the Maxwell–Boltzmann distribution if higher temperatures and lower particle densities are involved. In other words, we cannot seeĀ the Fermi-Dirac distributions (all matter is fermionic, except for weird stuff like superfluid helium-4 at 1 or 2 degrees Kelvin),Ā but they are there!

Let’s approach it mathematically: the most general formula, encompassing both Fermi-Dirac and Bose-Einstein statistics, is:

Ni(Ei) āˆ 1/[e(EiĀ āˆ’ μ)/kT ± 1]

If you’d google, you’d find a formula involving an additional coefficient, gi, which is the so-calledĀ degeneracyĀ of the energy level Ei. I included it in the formula I used in the above-mentioned post of mine. However, I don’t want to make it any more complicated than it already is and, therefore, I omitted it this time.Ā What you need to look at are the two terms in the denominator: e(EiĀ āˆ’ μ)/kTĀ and ± 1.

From a math point of view, it is obvious that the values of e(EiĀ āˆ’ μ)/kTĀ + 1 (Fermi-Dirac) and e(EiĀ āˆ’ μ)/kTĀ āˆ’ 1 (Bose-Einstein) will approach each other if e(EiĀ āˆ’ μ)/kTĀ is muchĀ larger than ±1, so if e(EiĀ āˆ’ μ)/kTĀ >>Ā 1. That’s the case, obviously, if the (EiĀ āˆ’ μ)/kT ratio is large, so if (EiĀ āˆ’ μ)Ā >> kT. In fact, (EiĀ āˆ’ μ) should, obviously, be much larger than kT for the lowestĀ energy levels too!Ā Now, the conditions under which that is the case are associated with the classical situation (such as a cylinder filled with gas, for example). Why?

Well… […] Again, I have to say that this blog can’t substitute for a proper textbook. Hence, I am afraid I have to leave it to you to do the necessary research to see why. šŸ™‚Ā The non-mathematical approach is to simple note that quantum effects, i.e. the ±1 term, only apply if the concentration of particles is high enough. Indeed, quantum effects appear if the concentration of particles is higher than the so-called quantum concentration. Only when the quantum concentration is reached, particles will start interacting according to what they are, i.e. as bosons or as fermions. At higher temperature, that concentration willĀ notĀ be reached, except in massive objects such as aĀ white dwarfĀ (white dwarfs are stellar remnants with the mass like that of the Sun but a volume like that of the Earth). So, in general, we can say that at higher temperatures and at low concentration we will not have any quantum effects. That should settle the matter—as for now, at least.

You’ll have one last question: we derived Boltzmann’s Law from the kinetic theory of gases, but how do we derive that Ni(Ei) = 1/[Ae(EiĀ āˆ’ μ)/kT ± 1] expression? Good question but, again, we’d need more than a few pages to explain that! The answer is: quantum mechanics, of course! Go check it out in Feynman’s third Volume of Lectures! šŸ™‚

Post scriptum: combinations, permutations and multiplicity

The mentioned example fromĀ HyperPhysicsĀ is really interesting, if only because it shows you also need to master a bit of combinatorics to get into quantum mechanics. Let’s go through the basics. If we have n distinctĀ objects, we can order hem in n! ways, with n!Ā (read: n factorial) equal to nĀ·(n–1)Ā·(n–2)Ā·…Ā·3Ā·2Ā·1. Note that 0! is equal to 1, per definition. We’ll need that definition.

For example, a red, blue and green ball can be ordered in 3Ā·2Ā·1 = 6 ways. Each way is referred to as aĀ permutation.

Besides permutations, we also have the concept of aĀ k-permutation, which we can denote in a number of ways but let’s choose P(n, k). [The P stands forĀ permutation here, not for probability.] P(n, k) is the number of ways to pick k objects out of a set of n objects. Again, the objects are supposed to be distinguishable. The formula is P(n, k) = nĀ·(n–1)Ā·(n–2)Ā·…Ā·(n–k+1) = n!/(n–k)!.Ā That’s easy to understand intuitively: on your first pick you have n choices; on your second, n–1; on your third, n–2, etcetera. When n = k, we obviously get n! again.

There is a third concept: the k-combinationĀ (as opposed to the k-permutation), which we’ll denote by C(n, k). That’s when the order withinĀ our subsetĀ doesn’t matter: an ace, a queen and a jack taken out of some card deck are a queen, a jack, and an ace: we don’t care about the order. If we have k objects, there are k! ways of ordering them and, hence, we just have to divide P(n, k) by k! to get C(n, k). So we write: C(n, k) = P(n, k)/k! = n!/[(n–k)!k!]. You recognize C(n, k): it’s the binomial coeficient.

Now, the HyperPhysicsĀ example illustrating the three mentioned distributions (Maxwell-Boltzmann, Bose-Einstein and Fermi-Dirac) is a bit more complicated: we need to associate q energy levels with N particles. Every possible configuration is referred to as a micro-state, and the total number of possible micro-states is referred to as the multiplicity of the system, denoted by Ī©(N, q). The formula for Ī©(N, q) is another binomial coefficient: Ī©(N, q) = (q+N–1)!/[q!(N–1)!]. Ī©(N, q) = Ī©(6, 9) = (9+6–1)!/[9!(6–1)!] = 2002.

In our example, however, we do not have distinct particles and, therefore, we only have 26 macro-states (as opposed to 2002 micro-states), which are also referred to, confusingly, asĀ distributionsĀ or combinations.

Now, the number of micro-states associated with the same macro-state is given by yet another formula: it is equal to N!/[n1!Ā·n2!Ā·n3!Ā·…Ā·nq!], with ni! the number of particles in level i. [See why we need the 0! = 1 definition? It ensures unoccupied states do not affect the calculation.] So that’s how we get those numbersĀ 6, 60 and 180 for those three macro-states.

But how do we calculate those average numbers of particles for each energy level? In other words, how do we calculate the probability densities under the Maxwell-Boltzmann, Fermi-Dirac and Bose-Einstein hypothesis respectively?

For the Maxwell-Boltzmann distribution, we proceed as follows: for each energy level j (or Ej, I should say), we calculate njĀ = āˆ‘nijĀ·PiĀ over all macro-states i.Ā In this summation, we have nij, which is the number of particles in energy level j in micro-state i, while PiĀ is the probability of macro-state i as calculated by the ratio of (i) the number of micro-states associated with macro-state i and (ii) the total number of micro-states. For Pi, we gave the example of 3/2002 ā‰ˆ 0.3%. For 60 and 180, we get 60/2002 ā‰ˆ 3% and 180/2002 ā‰ˆ 9%. Calculating all the nj‘s for j ranging from 1 to 9 should yield the numbers and the graph below indeed.

M-B graphOK. That’s how it works for Maxwell-Boltzmann. Now, it is obvious that the Fermi-Dirac and the Bose-Einstein distribution should notĀ be calculated in the same way because, if they were, they would not be different from the Maxwell-Boltzmann distribution! The trick is as follows.

For the Bose-Einstein distribution, we give all macro-states equal weight—so that’s a weight of one, as shown below. Hence, the probability PiĀ  is, quite simply, 1/26Ā ā‰ˆ 3.85%Ā for all 26 macro-states. So we use the sameĀ njĀ = āˆ‘nijĀ·PiĀ formula but with PiĀ = 1/26.

BE

Finally, I already explained how we get the Fermi-Dirac distribution: we can only have (i) one, (ii) two, or (iii) zeroĀ fermions for each energy level—not more than two! Hence, out of the 26 macro-states, only five are actually possible under the Fermi-Dirac hypothesis, as illustrated below once more.Ā So it’s a very different distribution indeed!

Table 3

Now, you’ll probably still have questions. For example, why does the assumption, for the Bose-Einstein analysis, that macro-states have equal probability favor the lower energy states? The answer is that the model also integrates other constraints: first, when associating a particle with an energy level, we doĀ notĀ favor one energy level over another, so all energy levels have equal probability. However, at the same time, the whole system has someĀ fixedĀ energy level, and so we cannot put the particles in the higher energy levels only! At the same time, we know that, if we have q particles, and the probability of a particle having some energy level j is the same for all j, then they are likelyĀ notĀ to be all at the same energy level: they’ll be distributed, effectively, as evidenced by the very low chance (0.3% only) of having 5 particles in the ground state and 1 particle at a higher level, as opposed to the 3% and 9% chance of the other two combinations shown in that diagram with three possible Maxwell-Boltzmann (MB) combinations.

So what happens when assigning anĀ equalĀ probability to all 26 possible combinations (with value 1/26) is that the combinations that were previously rather unlikely – because they did have a rather heavy concentration of particles in the ground state only – are now much moreĀ likely. So that’s why the Bose-Einstein distribution, in this example at least, is skewed towards the lowest energy level—as compared to the Maxwell-Boltzmann distribution, that is.

So that’s what’s behind, and that should also answer the other question you surely have when looking at those five acceptable Fermi-Dirac configurations: why don’t we have the same five configurations starting from the top down, rather than from the bottom up? Now you know: such configuration would have much higher energy overall, and so that’s not allowed under this particular model.

There’s also this other question: we said the particles were indistinguishable, but so then we suddenly say there can be two at any energy level, because their spin is opposite. It’s obvious this is ratherĀ ad hocĀ as well. However, if we’d allow only one particle at any energy level, we’d haveĀ noĀ allowable combinations and, hence, we’d have no Fermi-Dirac distribution at all in this example.

In short, the example is rather intuitive, which is actually why I like it so much: it shows how bosonic and fermionic behavior appear rather gradually, as a consequence ofĀ variables that are defined at the systemĀ level, such as density, or temperature. So, yes, you’re right if you think the HyperPhysicsĀ example lacks rigor. That’s whyĀ I think it’s such wonderful pedagogic device. šŸ™‚

The Quantum-Mechanical Gas Law

Pre-script (dated 26 June 2020): This post has become less relevant (even irrelevant, perhaps) because my views on all things quantum-mechanical have evolved significantly as a result of my progression towards a more complete realist (classical) interpretation of quantum physics. The text also got mutilated because of the removal of material by the dark force. I keep blog posts like these mainly because I want to keep track of where I came from. I might review them one day, but I currently don’t have the time or energy for it. šŸ™‚

Original post:

In my previous posts, it was mentioned repeatedly that the kinetic theory of gases isĀ notĀ quite correct: the experimentally measured values of the so-called specific heat ratioĀ (γ) vary with temperature and, more importantly, their values differ, in general, from what classical theory would predict. It works, more or less, for noble gases, which do behave as ideal gases and for which γ is what the kinetic theory of gases would want it to be: γ = 5/3—but we get in trouble immediately, even for simple diatomic gases like oxygen or hydrogen, as illustrated below: the theoretical value is 9/7 (so that’s 1.286, more or less), but the measured value is very different.

Heat ratioLet me quickly remind you how we get the theoretical number. According to classical theory, a diatomic molecule like oxygen can be represented as two atoms connected by a spring. Each of the atoms absorbs kinetic energy, and for each direction of motion (x, y and z), that energy is equal to kT/2, so the kinetic energy of both atoms – added together – is 2Ā·3Ā·kT/2 = 3kT. However, I should immediately add that not all of that energy is to be associated with the center-of-mass motion of the whole molecule, which determines the temperatureĀ of the gas: that energy is and remains equal to the 3kT/2, always. We also have rotational and vibratory motion. The molecule can rotate in two independent directions (and any combination of these directions, of course) and, hence, rotational motion is to absorb an amount of energy equal to 2Ā·kT/2 = kT. Finally, the vibratory motion is to be analyzed as any other oscillation, so like a spring really. There is only one dimension involved and, hence, the kinetic energy here is just kT/2. However, we know that the total energy in an oscillator is the sum of the kinetic and potential energy, which adds another kT/2 term. Putting it all together, we find that the average energy for each diatomic particle is (or should be) equal to 7Ā·kT/2 = (7/2)kT. Now, as mentioned above, theĀ temperature of the gas (T) is proportional to the mean molecular energy of the center-of-mass motion only (in fact, that’s how temperature isĀ defined), with the constant of proportionality equal to 3k/2. Hence, for monatomic ideal gases, we can write: U = NĀ·(3k/2)T and, therefore, PV = NkT = (2/3)Ā·U. Now, γ appears as follows in the ideal gas law:Ā PV = (γ–1)U. Therefore, γ = 2/3 + 1 = 5/3, but so that’sĀ for monatomic ideal gases only! The total kinetic energy of our diatomic molecule is U = NĀ·(7k/2)T and, therefore, PV = (2/7)Ā·U. So γ must be γ = 2/7 + 1 = 9/7 ā‰ˆ 1.286 for diatomic gases, like oxygen and hydrogen.

Phew! So that’s the theory. However, as we can see from the diagram, γ approaches that value only when we heat the gas to a few thousand degrees! So what’s wrong? One assumption is that certain kinds of motions “freeze out” as the temperature falls—although it’s kinda weird to think of something ‘freezing out’ at a thousand degrees Kelvin! In any case, at the end of the 19th century, that was the assumption that was advanced, very reluctantly, by scientists such as James Jeans. However, the mystery was about to be solved then, as Max Planck, even more reluctantly, presented his quantum theory of energy at the turn of the century itself.

But the quantum theory was confirmed and so we should now see how we can apply it toĀ the behavior of gas. In my humble view, it’s a really interesting analysis, because we’re applying quantum theory here to a phenomenon that’s usually being analyzed as a classical problem only.

Boltzmann’s Law

We derived Boltzmann’s Law in our post on the First Principles of Statistical Mechanics. To be precise, we gave Boltzmann’s Law for the density of a gas (which we denoted byĀ n = N/V) Ā in a force field, like a gravitational field, or in an electromagnetic field (assuming our gas particles are electrically charged, of course). We noted, however, Boltzmann’s Law was also applicable to much more complicated situations, like the one below, which shows a potential energy function for two molecules that is quite characteristic of the way molecules actually behave: when they come veryĀ close together, they repel each other but, at larger distances, there’s a force of attraction. We don’t really know the forces behind but we don’t need to: as long as these forces are conservative, they can combine in whatever way they want to combine, and Boltzmann’s Law will be applicable. [It should be obvious why. If you hesitate, just think of the definition of work and how it affects potential energy and all that. Work is force times distance, but when doing work, we’re also changing potential energy indeed! So if we’ve got a potential energy function, we can get all the rest.]

randomBoltzmann’s Law itself is illustrated by the graph below, which also gives the formula for it: n = n0Ā·eāˆ’P.E/kT.

graph

It’s a graph starting at n = n0Ā for P.E. = 0, and it then decreasesĀ exponentially. [Funny expression, isn’t it? So as to respect mathematical terminology, I should say that itĀ decaysĀ exponentially.] In any case, ifĀ anything, Boltzmann’s Law shows the natural exponential function is quite ‘natural’ indeed, because Boltzmann’s Law pops up in Nature everywhere! Indeed, Boltzmann’s Law is not limited to functions of potential energy only. For example, Feynman derives another Boltzmann Law for the distribution of molecular speeds or, so as to ensure the formula is also valid in relativity, the distribution of molecularĀ momenta. In case you forgot, momentum (p) is the product of mass (m) and velocity (u), and the relevant Boltzmann Law is:

f(p)Ā·dp = CĀ·eāˆ’K.E/kTĀ·dp

The argument is not terribly complicated but somewhat lengthy, and so I’ll refer you to the link for more details. As for the f(p) function (and the dp factor on both sides of the equation), that’s because we’re not talkingĀ exactĀ values of p but some range equal to dp and some probabilityĀ of finding particles that have a momentum within that range. The principle is illustrated below for molecular speeds (denoted by u = p/m), so we have a velocity distribution below. The illustration for p would look the same: just substitute u for p.

Distribution

Boltzmann’s Law can be stated, much more generally, as follows:

The probability of different conditions of energy (E), potential or kinetic, is proportional to eāˆ’E/kT.Ā 

As Feynman notes, “This is a rather beautiful proposition, and a very easy thing to remember too!”Ā It is, and we’ll need it for the next bit.

The quantum-mechanical theory of gases

According to quantum theory, energy comes inĀ discreteĀ packets, quanta, and any system, like an oscillator, will only have aĀ discrete set of energy levels, i.e. states of different energy. An energy state is, obviously, a condition of energy and, hence, Boltzmann’s Law applies. More specifically, if we denote the various energy levels, i.e. the energies of the various molecular states, by E0, E1, E2,…,Ā Ei,…, and if Boltzmann’s Law applies, then the probability of finding a molecule in the particular state EiĀ will be proportional toĀ eāˆ’EiĀ /kT.

Now, we know we’ve got some constant there, but we can get rid of that by calculating relative probabilities. For example, the probability of being in stateĀ E1, relative to the probability of being in state E0, is:

P1/P0Ā = eāˆ’E1Ā /kT/eāˆ’E0Ā /kTĀ = eāˆ’(E1–E0)/kT

But the relative probability P1Ā should, obviously, also be equal to the ratio n1/N, i.e. the ratio of the number of molecules in state E1Ā and the total number of molecules. Likewise, P0Ā = n0/N. Hence, P1/P0Ā = n1/n0Ā and, therefore, we can write:

n = n0eāˆ’(E1–E0)/kT

What can we do with that? Remember we want to explain the behavior of non-monatomic gas—like diatomic gas, for example. Now we need some other assumption, obviously. As it turns out, the assumption that we can represent a system as some kind of oscillation still makes sense! In fact, the assumption that our diatomic molecule is like a spring is equally crucial to our quantum-theoretical analysis of gases as it is to our classical kinetic theory of gases. To be precise, in both theories, we look at it as a harmonic oscillator.

Don’t panic. A harmonic oscillator is, quite simply, a system that, when displaced from its equilibrium position, experiences some kind of restoring force. Now, for it to be harmonic, the force needs to be linear. For example, when talking springs, the restoring force F will be proportionalĀ to the displacement x). It basically means we can use a linear differential equation to analyze the system, like mĀ·(d2x/dt2) = –kx. […]Ā I hope you recognize this equation, because you should! It’s Newton’s Law: F = mĀ·aĀ with F = –kĀ·x. If you remember the equation, you’ll also remember that harmonic oscillations were sinusoidal oscillations with a constantĀ amplitudeĀ and a constantĀ frequency. That frequency did not depend on theĀ amplitude: because of the sinusoidal function involved, it was easier to write that frequency as an angularĀ frequency, which we denoted by ω0Ā and which, in the case of our spring, was equal to ω0Ā = (k/m)1/2. So it’s a property of the system. Indeed, ω0Ā is the square root of the ratio of (1) k, which characterizes the spring (it’s its stiffness), and (2) m, i.e. the mass on the spring. Solving the differential equation yielded x = AĀ·cos(ω0t + Ī”) as a general solution, with A the (maximum) amplitude, and Ī” some phase shift determined by our tĀ = 0 point.Ā Let me quickly jot down too more formulas: the potential energy in the spring is kx2/2, while its kinetic energy is mv2/2,Ā as usual (so the kinetic energy depends on the mass and its velocity, while the potential energy only depends on the displacement and the spring’s stiffness). Of course, kinetic and potential energy add up to the totalĀ energy of the system, which is constant and proportional to the square of the (maximum) amplitude: K.E. + P.E. =Ā EĀ āˆ A2. To be precise, E = kA2/2.

That’s simple enough. Let’s get back to our molecularĀ oscillator. While the total energy of an oscillator in classical theory can take on any value, Planck challenged that assumption: according to quantum theory, it can only take up energies equal to ħω at a time. [Note that we use the so-called reduced Planck constant here (i.e. h-bar), because we’re dealing with angular frequencies.] Hence, according to quantum theory, we have an oscillator with equally spaced energy levels, and the difference between them is ħω. Now, ħω is terribly tiny—but it’s there. Let me visualize what I just wrote:

Equipartition-3

So our expression forĀ P1/P0Ā becomes P1/P0Ā =Ā eāˆ’Ä§Ļ‰/kT/eāˆ’0/kTĀ = eāˆ’Ä§Ļ‰/kT. More generally, we haveĀ Pi/P0Ā =Ā eāˆ’i·ħω/kT. So what? Well… We’ve got a function here which gives the chance of finding a molecule in state PiĀ relative to that of finding it in state E0, and it’s a function ofĀ temperature. Now, the graph below illustrates the general shape of that function. It’s a bit peculiar, but you can see that the relative probability goes up and down with temperature. The graph makes it clear that, at extremely low temperatures, most particles will be in state E0Ā and, of course, the internal energy of our body of gas will be close to nil.

Capture-2

Now, we can look at the oscillators in the bottom state (i.e. particles in the molecular energy state E0) as being effectively ‘frozen’: they don’t contribute to the specific heat. However, as we increase the temperature, our molecules gradually begin to have an appreciable probability to be in the second state, and then in the next state, and so on, and so the internal energy of the gas increases effectively. Now, when the probability is appreciable for many states, the quantized states become nearly indistinguishable and, hence, the situation is like classical physics: it is nearly indistinguishable from a continuumĀ of energies.

Now, while you can imagine such analysis should explain why the specific heat ratio for oxygen and hydrogen varies as it does in the very first graph of this post, you can also imagine the details of that analysis fill quite a few pages! In fact, even Feynman doesn’t include it in his Lectures. What he does include is the analysis of the blackbody radiation problem, which is remarkably similar. So… Well… For more details on that, I’ll refer you to Feynman indeed. šŸ™‚

I hope you appreciated this little ‘lecture’, as it sort of wraps up my ‘series’ of posts on statistical mechanics, thermodynamics and, central to both, the classical theory of gases. Have fun with it all!

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

Entropy, energy and enthalpy

Pre-script (dated 26 June 2020): This post has become less relevant (even irrelevant, perhaps) because my views on all things quantum-mechanical have evolved significantly as a result of my progression towards a more complete realist (classical) interpretation of quantum physics. The text also got mutilated because of the removal of material by the dark force. I keep blog posts like these mainly because I want to keep track of where I came from. I might review them one day, but I currently don’t have the time or energy for it. šŸ™‚

Original post:

Phew! I am quite happy I got through Feynman’s chapters on thermodynamics. Now is a good time to review the math behind it. We thoroughly understand the gas equation now:

PV = NkT = (γ–1)U

The gamma (γ) in this equation is the specific heat ratio: it’s 5/3 for ideal gases (so that’s about 1.667) and, theoretically, 4/3 ā‰ˆ 1.333 or 9/7 ā‰ˆ 1.286 for diatomic gases, depending on the degrees of freedom we associate with diatomic molecules. More complicated molecules have even more degrees of freedom and, hence, can absorb even more energy, so γ gets closer to one—according to the kinetic gas theory, that is. While we know that the kinetic gas theory is not quite accurate – an approach involving molecular energy states is a better match for reality – that doesn’t matter here. As for the term (specific heat ratio), I’ll explain that later. [I promise. šŸ™‚ You’ll see it’s quite logical.]

The point to note is that this body of gas (or whatever substance) stores an amount of energy U that is directly proportional to the temperature (T), and Nk/(γ–1) is the constant of proportionality. We can also phrase it the other way around: the temperature is directly proportional to the energy, with (γ–1)/Nk the constant of proportionality. It means temperature and energy are in a linear relationship. [Yes, direct proportionality implies linearity.] The graph below shows the T = [(γ–1)/Nk]Ā·U relationship for three different values of γ, ranging from 5/3 (i.e. the maximum value, which characterizes monatomic noble gases such as helium, neon or krypton) to a value close to 1, which is characteristic of more complicated molecular arrangements indeed, such as heptane (γ = 1.06) or methyl butane ((γ = 1.08). The illustration shows that, unlike monatomic gas, more complicated molecular arrangements allow the gas to absorb a lot of (heat) energy with a relatively moderate rise in temperature only.

CaptureWe’ll soon encounter another variable, enthalpy (H), which is also linearly related to energy: H = γU. From a math point of view, these linear relationships don’t mean all that much: they just show these variables – temperature, energy and enthalphy – are all directly related and, hence, can be defined in terms of each other.

We can invent other variables, like the Gibbs energy, or the Helmholtz energy. In contrast, entropy, while often being mentioned as just some other state function, is something different altogether. In fact, the term ‘state function’ causes a lot of confusion: pressure and volume are state variables too. The term is used to distinguish these variables from so-called process functions, notably heat and work. Process functions describe how we go from one equilibrium state to another, as opposed to the state variables, which describe the equilibrium situation itself. Don’t worry too much about the distinction—for now, that is.

Let’s look at non-linear stuff. The PV = NkT = (γ–1)U says thatĀ pressure (P) and volume (V) are inversely proportional one to another, and so that’s a non-linear relationship. [Yes, inverseĀ proportionality is non-linear.] To help you visualize things, I inserted a simple volume-pressure diagram below, which shows how pressure and volume are related for three different values of U (or, what amounts to the same, three different values of T).

graph 2

The curves are simple hyperbolas which have the x- and y-axis as horizontal and vertical asymptote respectively. If you’ve studied social sciences (like me!) – so if you know a tiny little bit of the ‘dismal science’, i.e. economics (like me!) – you’ll note they look like indifference curves. The x- and y-axis then represent the quantity of some good X and some good Y respectively, and the curves closer to the origin are associated with lower utility. How much X and Y we will buy then, depends on (a) their price and (b) our budget, which we represented by a linear budget line tangent to the curve we can reach with our budget, and then we are a little bit happy, very happy or extremely happy, depending on our budget. Hence, our budget determines our happiness. From a math point of view, however, we can also look at it the other way around: our happiness determines our budget. [NowĀ that‘s a nice one, isn’t it? Think about it! šŸ™‚ And, in the process, think about hyperbolas too: the y = 1/x function holds the key to understanding both infinity and nothingness. :-)]

U is a state function but, as mentioned above, we’ve got quite a few state variables in physics. Entropy, of course, denoted by S—and enthalpy too, denoted by H. Let me remind you of the basics of theĀ entropy concept:

  1. The internal energy U changes because (a) we add or remove some heat from the system (Ī”Q), (b) because some work is being done (by the gas on its surroundings or the other way around), or (c) because of both. Using the differential notation, we write: dU = dQ – dW,Ā always. The (differential) work that’s being done is PdV. Hence, we have dU = dQ – PdV.
  2. When transferring heat to a system at a certain temperature, there’s a quantity we refer to as the entropy. Remember that illustration of Feynman’s in my post on entropy: we go from one point to another on the temperature-volume diagram, taking infinitesimally small steps along the curve, and, atĀ each step, an infinitesimal amount of work dW is done, and an infinitesimal amount of entropy dS = dQ/T is being delivered.
  3. The total change in entropy, Ī”S, is a line integral: Ī”S = ∫LĀ dQ/T = ∫LĀ dS.

That’s somewhat tougher to understand than economics, and so that’s why it took me more time to come with terms with it. šŸ™‚ Just go through Feynman’s LectureĀ on it, or through that post I referenced above. If you don’t want to do that, then just note that, while entropy is a very mysterious concept, it’s deceptively simple from a math point of view: Ī”S = Ī”Q/T, so the (infinitesimal) change in entropy is, quite simply, the ratio of (1) the (infinitesimal or incremental) amount of heat that is being added or removed as the system goes from one state to another through a reversible processĀ and (2) the temperature at which the heat is being transferred. However, I am not writing this post to discuss entropy once again. I am writing it to give you an idea of the math behind the system.

SoĀ dS = dQ/T. Hence, we can re-write dU = dQ – dW as:

dU = TdS – PdV ⇔ dU + d(PV) = TdS – PdV + d(PV)

⇔ d(U + PV) = dH = TdS – PdV + PdV + VdP = TdS + VdP

The U + PV quantity on the left-hand side of the equation is the so-called enthalpy of the system, which I mentioned above. It’s denoted by H indeed, and it’s just another state variable, like energy: same-same but different, as they say in Asia. We encountered it in our previous post also, where we said that chemists prefer to analyze the behavior of substances using temperature and pressure as ‘independent variables’, rather than temperature and volume. Independent variables? What does that mean, exactly?

According to the PV = NkT equation, we only have two independent variables: if we assign some value to two variables, we’ve got a value for the third one. Indeed, remember that other equation we got when we took theĀ totalĀ differential of U. WeĀ wrote U as U(V, T) and, taking the total differential, we got:

dU = (āˆ‚U/āˆ‚T)dT + (āˆ‚U/āˆ‚V)dV

We did not need to add a (āˆ‚U/āˆ‚P)dP term, because the pressure is determined by the volume and the temperature. We could also have writtenĀ U = U(P, T) and, therefore, thatĀ dU = (āˆ‚U/āˆ‚T)dT + (āˆ‚U/āˆ‚P)dP. However, when working with temperature and pressure as the ‘independent’ variables, it’s easier to work with H rather than U. The point to note is that it’s all quite flexible really: we have two independent variables in the system only. TheĀ third one (and all of the other variables really, like energy or enthalpy or whatever) depend on the other two. In other words, from a math point of view, we only have two degrees of freedomĀ in the system here: only two variables are actually free to vary. šŸ™‚

Let’s look at that dH = TdS + VdP equation. That’s a differential equation in which not temperature and pressure, but entropy (S) and pressure (P) are ‘independent’ variables, so we write:

dH(S, P) =Ā TdS + VdP

Now, it is not very likely that we will have some problem to solve with data on entropy and pressure. At our level of understanding, any problem that’s likely to come our way will probably come with data on more common variables, such as the heat, the pressure, the temperature, and/or the volume. So we could continue with the expression above but we don’t do that. It makes more sense to re-write the expression substituting TdS for dQ once again, so we get:

dH = dQ + VdP

That resembles our dU = dQ – PdV expression: it just substitutes V for –P. And, yes, you guessed it: it’s because the two expressions resemble each other that we like to work with H now. šŸ™‚ Indeed, we’re talking the same system and the same infinitesimal changes and, therefore, we can use all the formulas we derived already by just substituting H for U, V for –P, and dP for dV. Huh?Ā Yes. It’s a rather tricky substitution. If we switch V for –P (or vice versa) in a partial derivative involving T, we also need to include the minus sign. However, we do not need to include the minus sign when substituting dV and dP, and we also don’t need to change the sign of the partial derivatives of U and H when going from one expression to another! It’s a subtle and somewhat weird point, but a very important one! I’ll explain it in a moment. Just continue to read as for now. Let’s do the substitution using our rules:

dU = (āˆ‚Q/āˆ‚T)VdT + [T(āˆ‚P/āˆ‚T)VĀ āˆ’ P]dV becomes:

dH = (āˆ‚Q/āˆ‚T)PdT + (āˆ‚H/āˆ‚P)TdP =Ā CPdT + [–TĀ·(āˆ‚V/āˆ‚T)P + V]dP

Note that, just as we referred to (āˆ‚Q/āˆ‚T)VĀ as the specific heat capacity of a substance at constant volume, which we denoted byĀ CV, we now refer toĀ (āˆ‚Q/āˆ‚T)PĀ as the specific heat capacityĀ at constant pressure, which we’ll denote, logically, as CP. Dropping the subscripts of the partial derivatives, we re-write the expression above as:

dH = CPdT + [–TĀ·(āˆ‚V/āˆ‚T)Ā + V]dP

So we’ve got what we wanted: we switched from an expression involving derivatives assuming constant volume to an expression involving derivatives assuming constant pressure. [In case you wondered what we wanted, this is it: we wanted an equation that helps us to solve another type of problem—another formula for a problem involving a different set of data.]

As mentioned above, it’s good to use subscripts with the partial derivatives to emphasize what changes and what is constant when calculating those partial derivatives but, strictly speaking, it’s not necessary, and you will usually notĀ find the subscripts when googling other texts. For example, inĀ the Wikipedia article on enthalpy, you’ll find the expression written as:

dH = CPdT + V(1–αT)dP with α = (1/V)(āˆ‚V/āˆ‚T)

Just write it all out and you’ll find it’s the same thing, exactly. It just introduces another coefficient, α, i.e. the coefficient of (cubic) thermal expansion. If you find this formula is easier to remember, then please use this one. It doesn’t matter.

Now, let’s explain that funny business with the minus signs in the substitution. I’ll do so by going back to that infinitesimal analysis of the reversible cycle in my previous post, in which we had that formula involving Ī”QĀ for the work done by the gas during an infinitesimally small reversible cycle:Ā Ī”W = Ī”VĪ”P = Ī”QĀ·(Ī”T/T). Now, we can either write that as:

  1. Ī”Q = TĀ·(Ī”P/Ī”T)Ā·Ī”V = dQ = TĀ·(āˆ‚P/āˆ‚T)VĀ·dV – which is what we did for our analysis of (āˆ‚U/āˆ‚V)T – or, alternatively, as
  2. Ī”Q = TĀ·(Ī”V/Ī”T)Ā·Ī”P = dQ =Ā TĀ·(āˆ‚V/āˆ‚T)PĀ·dP, which is what we’ve got to do here, for our analysis of (āˆ‚H/āˆ‚P)T.

Hence,Ā dH = dQ + VdP becomes dH =Ā TĀ·(āˆ‚V/āˆ‚T)PĀ·dP + VĀ·dP, and dividing all by dP gives us what we want to get: dH/dP = (āˆ‚H/āˆ‚P)TĀ = TĀ·(āˆ‚V/āˆ‚T)PĀ + V.

[…]Ā Well… NO! We don’t have the minus sign in front of TĀ·(āˆ‚V/āˆ‚T)P, so we must have done something wrong or, else, that formula above is wrong.

The formula is right (it’s in Wikipedia, so it must be right :-)), so we are wrong. Indeed! The thing is: substituting dT, dV and dP for Ī”T, Ī”V and Ī”P is somewhat tricky.Ā The geometric analysis (illustrated below) makes sense but we need to watch the signs.

Carnot 2

We’ve got a volume increase, a temperature drop and, hence, also a pressure drop over the cycle: the volume goes from V to V+Ī”V (and then back to V, of course), while the pressure and the temperature go from P to P–ΔP and T to T–ΔT respectively (and then back to P and T, of course). Hence, we should write: Ī”V = dV, –ΔT = dT, and –ΔP = dP. Therefore, as we replace the ratio of the infinitesimal change of pressure and temperature, Ī”P/Ī”T,Ā by a proper derivative (i.e. āˆ‚P/āˆ‚T), we should add a minus sign: Ī”P/Ī”T = ā€“āˆ‚P/āˆ‚T. Now that gives us what we want:Ā dH/dP = (āˆ‚H/āˆ‚P)TĀ = –TĀ·(āˆ‚V/āˆ‚T)PĀ + V, and, therefore,Ā we can, indeed, write what we wrote above:

dU = (āˆ‚Q/āˆ‚T)VdT + [T(āˆ‚P/āˆ‚T)VĀ āˆ’ P]dV becomes:

dH = (āˆ‚Q/āˆ‚T)PdT + [–TĀ·(āˆ‚V/āˆ‚T)P + V]dP =Ā CPdT + [–TĀ·(āˆ‚V/āˆ‚T)P + V]dP

Now, in case you still wonder: what’s the use of all these different expressions stating the same? The answer is simple: it depends on the problem and what information we have. Indeed, note that all derivatives we use in our expression for dH expression assume constant pressure, so ifĀ we’ve got that kind of data, we’ll use the chemists’ representation of the system. If we’ve got data describing performance at constant volume,Ā we’ll need the physicists’ formulas, which are given in terms of derivatives assuming constant volume. It all looks complicated but, in the end, it’s the same thing: theĀ PV = NkT equation gives us two ‘independent’ variables and one ‘dependent’ variable. Which one is which will determine our approach.

Now, we left one thing unexplained. Why do we refer to γ as the specific heat ratio? The answer is: it is the ratio of the specific heat capacities indeed, so we can write:

γ = CP/CV

However, it is important to note that that’s valid for ideal gases only. In that case, we know that the (āˆ‚U/āˆ‚V)PĀ derivative in ourĀ dU = (āˆ‚U/āˆ‚T)VdT + (āˆ‚U/āˆ‚V)TdV expression is zero: we can change the volume, but if the temperature remains the same, the internal energy remains the same. Hence, dU = (āˆ‚U/āˆ‚T)VdT = CVdT, and dU/dT = CV. Likewise, the (āˆ‚H/āˆ‚P)TĀ derivative in ourĀ dH = (āˆ‚H/āˆ‚T)PdT + (āˆ‚H/āˆ‚P)TdP expression is zero—for ideal gases, that is. Hence, dH = (āˆ‚H/āˆ‚T)PdT =Ā CPdT, and dH/dT = CP. Hence,

CP/CVĀ = (dH/dT)/(dU/dT) = dH/dU

Does that make sense? If dH/dU = γ, then H must be some linear function of U. More specifically, H mustĀ be some function H = γU + c, with c some constant (it’s the so-called constant of integration). Now, γ is supposed to be constant too, of course. That’s all perfectly fine: indeed, combining the definition of H (H = U + PV), and using the PV = (γ–1)U relation, we have H = U + (γ–1)U = γU (hence,Ā c = 0). So, yes, dH/dU = γ, and γ = CP/CV.

Note the qualifier, however: we’re assuming γ is constant (which does notĀ imply the gas has to be ideal, so the interpretation is less restrictive than you might think it is). If γ isĀ not a constant,Ā it’s a different ballgame. […] So… Is γ actually constant? The illustration below shows γ is not constant for common diatomic gases like hydrogen or (somewhat less common) oxygen. It’s the same for other gases: when mentioning γ, we need to state the temperate at which we measured it too. 😦 Ā However, the illustration also shows the assumption of γ being constant holds fairly well if temperature varies only slightly (like plus or minus 100° C), so that’s OK. šŸ™‚

Heat ratio

I told you so: the kinetic gas theory is not quite accurate. An approach involving molecular energy states works much better (and is actually correct, as it’s consistent with quantum theory). But so we are where we are and I’ll save the quantum-theoretical approach for later. šŸ™‚

So… What’s left? Well… If you’dĀ googleĀ the Wikipedia article on enthalphy in order to check if I am not writing nonsense, you’ll find it gives γ as the ratio of H and U itself: γ = H/U. That’s not wrong, obviously (γ = H/U = γU/U = γ), but that formula doesn’t really explain why γ is referred to as the specific heat ratio, which is what I wanted to do here.

OK. We’ve covered a lot of ground, but let’s reflect some more. We did notĀ say a lot about entropy, and/orĀ the relation between energy and entropy. Too bad… The relationship between entropy and energy is obviouslyĀ notĀ so simple as between enthalpy and energy. Indeed, because of that easy H = γU relationship, enthalpy emerges as just some auxiliary variable: some temporary variable we need to calculate something. Entropy is, obviously, something different. Unlike enthalpy, entropy involves very complicated thinking, involving (ir)reversibility and all that. So it’s quite deep, I’d say – but I’ll write more about that later. I think this post has gone as far as it should. šŸ™‚

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

The Ideal versus the Actual Gas Law

Pre-script (dated 26 June 2020): This post has become less relevant (even irrelevant, perhaps) because my views on all things quantum-mechanical have evolved significantly as a result of my progression towards a more complete realist (classical) interpretation of quantum physics. The text also got mutilated because of the removal of material by the dark force. I keep blog posts like these mainly because I want to keep track of where I came from. I might review them one day, but I currently don’t have the time or energy for it. šŸ™‚

Original post:

In previous posts, we referred, repeatedly, to the so-called ideal gas law, for which we have various expressions. The expression we derived from analyzing the kinetics involved when individual gas particles (atoms or molecules) move and collide was PĀ·V = NĀ·kĀ·T, in which the variables are P (pressure), V (volume), N (the number of particles in the given volume), T (temperature) and k (the Boltzmann constant). We also wrote it as PĀ·V = (2/3)Ā·U, in which U represents the total energy, i.e. the sum of the energies of all gas particles.Ā We also said the PĀ·V = (2/3)Ā·U formula was only valid for monatomic gases, in which case U is the kinetic energy of the center-of-mass motion of the atoms.

In order to provide some more generality, the equation is often written as PĀ·V = (γ–1)Ā·U. Hence, for monatomic gases, we have γ = 5/3.Ā For a diatomic gas, we’ll also have vibrational and rotational kinetic energy. As we pointed out in a previous post, each independent direction of motion, i.e. each degree of freedomĀ in the system,Ā will absorb an amount of energy equal to kĀ·T/2. For monatomic gases, we have three independent directions of motion (x, y, z) and, hence, the total energy U = 3Ā·kĀ·T/2 = (2/3)Ā·U.

Finally, when we’re considering adiabatic expansion/compression only – so when we do not add or remove any heat to/from to the gas – we can also write the ideal gas law as PVγ = C, with C some constant. [It is important to note that this PVγ = C relation can be derived from the more generalĀ PĀ·V = (γ–1)Ā·U expression, but that the two expressions are not equivalent. Please have a look at the P.S. to this post on this, which shows how we get thatĀ PVγ = constant expression, and talks a bit about its meaning.]

So what’s the gas law for diatomic gas, like O2, i.e. oxygen? The key to the analysis of diatomic gases is, basically, a model which represents the oxygen molecule as two atoms connected by a spring, but with a force law that’s not as simplistic asĀ Hooke’s law: we’re not looking at some linear force, but a force that’s referred to as aĀ van der Waals force. The image below gives a vague idea of what that might imply. Remember: when moving an object in a force field, we change its potential energy, and the work done, as we move with or against the force, is equal to theĀ changeĀ in potential energy. The graph below shows the force is anything but linear.

randomThe illustration above is a graph of potential energy for two molecules, but we can also apply it for the ‘spring’ model for two atoms withinĀ a single molecule. ForĀ the detail, I’ll refer you to Feynman’s Lecture on this. It’s not that the full story is too complicated: it’s just too lengthy to reproduce it in this post. Just note the key point of the whole story: one arrives at a theoretical value for γ that is equal to γ = 9/7Ā ā‰ˆ 1.286.Ā Wonderful! Yes. Except for the fact that value does not correspond to what is measured in reality: the experimentally confirmed value for γ for oxygen (O2) is about 1.40.

What about other gases?Ā When measuring the value for other diatomic gases, like iodine (I2) or bromine (Br2), we get a value closer to the theoretical value (1.30 and 1.32 respectively) but, still, there’s a variation to be explained here. The value for hydrogen H2Ā is about 1.4, so that’s like oxygen again. For other gases, we again get different values. Why?Ā What’s the problem?

It cannot be explained using classical theory. In addition, doing the measurements for oxygen and hydrogen at various temperatures also reveals that γ is a function of temperature, as shown below. Now that’s another experimental fact that does notĀ line up with our kinetic theory of gases!

Heat ratioReality is right, always. Hence, our theory must be wrong. Our analysis of the independent direction of motions inside of a molecule doesn’t work—even for the simple case of a diatomic molecule. Great minds such as James Clerk Maxwell couldn’t solve the puzzle in the 19th century and, hence, had to admit classical theory was in trouble. Indeed, popular belief has it that the black-body radiation problem was the onlyĀ thing classical theory couldn’t explain in the late 19th century but that’s not true: there were many more problems keeping physicists awake. But so we’ve got a problem here. As Feynman writes:Ā “We might try some force law other than a spring but it turns out that anything else will only make γ higher. If we include more forms of energy, γ approaches unity more closely, contradicting the facts. All the classical theoretical things that one can think of will only make it worse. The fact is that there are electrons in each atom, and we know from their spectra that there are internal motions; each of the electrons should have at leastĀ kT/2 of kinetic energy, and something for the potential energy, so when these are added in, γ gets still smaller. It is ridiculous. It is wrong.”

So what’s the answer? The answer is to be found in quantum mechanics. Indeed, one can develop a model distinguishing various molecular statesĀ with various energy levels E0,Ā E1,Ā E2,…,Ā Ei,…, and then associate a probability distribution which gives us the probability of finding a molecule in a particular state. Some more assumptions, all quite similar to the assumptions used by Planck when he solved the black-body radiation problem, then give us what we want: to put it simply, it is like some of the motions ‘freeze out’ at lower temperatures. As a result, γ goes up as we go down in temperature.

Hence, quantum mechanics saves the day, again.Ā However, that’s not what I want to write about here. What I want to do here is to give you an equation for the internal energy of a gas which is based on what we can actually measure, so that’s pressure, volume and temperature. I’ll refer to it as the ActualĀ Gas Law, because it takes into account that γ is not someĀ fixed value (so it’s not some natural constant, like Planck’s or Boltzmann’s constant), and it also takes into account that we’re not always gas—ideal or actual gas—but also liquids and solids.

Now, we have many inter-connected variables here, and so the analysis is quite complicated. In fact, it’s a great opportunity to learn more about partial derivatives and how we can use them. So the lesson is as much about math as it about physics. In fact, it’s probably more about math. šŸ™‚ Let’s see what we can make out of it.

Energy, work, force, pressure and volume

First, I should remind you that work is something that is done by a force on some object in the direction of the displacement of that object. Hence, work is force times distance. Now, because the force may actually vary as our object is being displaced and while the work is being done, we represent work as a line integral:

W = ∫F·ds

We write F and s in bold-face and, hence, we’ve got a vector dot productĀ here, which ensures we only consider the component of the force in the direction of the displacement: FĀ·Ī”sĀ =Ā |F|Ā·|Ī”s|Ā·cosĪø, with Īø the angle between the force and the displacement.

As for the relationship between energy and work, you know that one: as we do work on an object, we change its energy, and that’s what we are looking at here: the (internal) energy of our substance. Indeed, when we have a volume of gas exerting pressure, it’s the same thing: some force is involved (pressure is the force per unit area, so we write: P = F/A) and, using the model of the box with the frictionless piston (illustrated below), we write:

dW = F(–dx) = – PAdx = – PdV

gas-pressure

The dW = – PdV formula is the one we use when looking atĀ infinitesimalĀ changes. When going through the full thing, we should integrate, as the volume (and the pressure) changes over the trajectory, so we write:

W = ∫PdV

Now, it is veryĀ important to note that the formulas above (dW = – PdV andĀ W = ∫PdV) are alwaysĀ valid. Always? Yes. We don’t care whether or not the compression (or expansion) is adiabatic or isothermal. [To put it differently, we don’t care whether or not heat is added to (or removed from) the gas as it expands (or decreases in volume).] We also don’t keep track of the temperature here. It doesn’t matter. Work is work.

Now, as you know, an integral is some area under a graph so I can rephrase our result as follows: the work that is being done by a gas, as it expands (or the work that we need to put in in order to compress it), is the area under the pressure-volume graph, always.

Of course, as we go through a so-called reversible cycle, getting work out of it, and then putting some work back in, we’ll have some overlapping areas cancelling each other. That’s how we derived the amount ofĀ usefulĀ (i.e.Ā net) work that can be done by an ideal gas engine (illustrated below) as it goes through a Carnot cycle, taking in some amount of heat Q1Ā from one reservoir (which is usually referred to as the boiler)Ā and delivering some other amount of heat (Q1) to another reservoir (usually referred to as the condenser). As I don’t want to repeat myself too much, I’ll refer you to one of my previous posts for more details. Hereunder, I just present the diagram once again. If you want to understand anything of what follows, you need to understand it—thoroughly.

Carnot cycle graphIt’s important to note that work is being done in each of the four steps of the cycle, and that the work done by the gas is positive when it expands, and negative when its volume is being reduced. So, let me repeat: the W = ∫PdV formula is valid for both adiabatic as well as isothermal expansion/compression. We just need to be careful about the sign and see in which direction it goes. Having said that, it’s obvious adiabatic and isothermal expansion/compression are two very different things and, hence, their impact on the (internal) energy of the gas is quite different:

  1. Adiabatic compression/expansion assumes that no (external) heat energy (Q) is added or removed and, hence,Ā all the work done goes into changing the internal energy (U). Hence, we can write: W = PĪ”V = –ΔU and, therefore, Ī”U = –PĪ”V. Of course, adiabatic compression/expansion must involve a change in temperature, as the kinetic energy of the gas molecules is being transferred from/to the piston. Hence, the temperatureĀ (which is nothing but the average kinetic energy of the molecules)Ā changes.
  2. In contrast, isothermal compression/expansion (i.e. a volume changeĀ without any change in temperature) must involve an exchange of heat energy with the surroundings so to allow the temperature to remain constant. So Ī”Q ≠ 0 in this case.

The grand but simple formula capturing all is, obviously:

Ī”U = Ī”Q – PĪ”V

It says what we’ve said already: the internal energy of a substance (a gas) changes because some work is being done as its volume changes and/or because some heat is added or removed.

Now we have to get serious about partial derivatives, which relate one variable (the so-called ‘dependent’ variable) to another (the ‘independent’ variable). Of course, in reality, all depends on all and, hence, the distinction is quite artificial. Physicists tend to treat temperature and volume as the ‘independent’ variables, while chemists seem to prefer to think in terms of pressure and temperature. In math, it doesn’t matter all that much: we simply take the reciprocal and there you go: dy/dx = 1/(dx/dy). We go from one to another. Well… OK… We’ve got a lot of variables here, so… Yes. You’re right. It’s not going to be that simple, obviously! šŸ™‚

Differential analysis

If we have some function f in two variables, x and y, then we can write:Ā Ī”f = f(x +Ā Ī”x, y +Ā Ī”y) – Ā f(x, y). We can then write the following clever thing:

partial derivativeWhat’s being said here is that we can approximateĀ Ī”f using the partialĀ derivativesĀ āˆ‚f/āˆ‚xĀ and āˆ‚f/āˆ‚y. Note that the formula above actually implies that we’re evaluating the (partial)Ā āˆ‚f/āˆ‚x derivative at point (x, y+Ī”y), rather than the pointĀ (x, y) itself. It’s a minor detail, but I think it’s good to signal it: this ‘clever thing’ is just pedagogical. [Feynman is the greatest teacher of all times! :-)] The mathematically correct approach is to simply give the formal definition of partial derivatives, and then just get on with it:

Partial derivative definitionNow, let us apply thatĀ Ī”f formula to what we’re interested in, and that’s the change in the (internal) energy U. So we write:

formula 1Now, we can’t do anything with this, in practice,Ā because we cannot directly measure the two partial derivatives. So, while this is an actualĀ gas law (which is what we want), it’s not aĀ practicalĀ one, because we can’t use it. šŸ™‚Ā Let’s see what we can do about that. We need to find some formula for those partial derivatives. Let’s have a look at theĀ (āˆ‚U/āˆ‚T)VĀ factor first. That factor is defined and referred to as the specific heat capacity at constant volume, and it’s usually denoted by CV. Hence, we write:

CVĀ = specific heat capacity at constant volume = (āˆ‚U/āˆ‚T)V

Heat capacity? But we’re talking internal energy here? It’s the same. Remember thatĀ Ī”U = Ī”Q – PĪ”V formula: if we keep the volume constant, then Ī”V = 0 and, hence, Ī”U = Ī”Q. Hence, all of the change in internal energy (and I really mean allĀ of the change) is the heat energy we’re adding or removing from the gas. Hence, we can also writeĀ CVĀ in its more usual definitional form:

CVĀ = (āˆ‚Q/āˆ‚T)V

As for its interpretation, you should look at it as a ratio: CVĀ is the amount of heat one must put into (or remove from) a substance in order to change its temperature by one degree with the volume held constant. Note that the term ‘specific heat capacity’ is usually referred to as the ‘specific heat’, as that’s shorter and simpler. However, you can see it’s some kind of ‘capacity’ indeed. More specifically, it’s a capacity of a substance to absorbĀ heat. Now that’s stuff we can actually measure and, hence, we’re done with the first term in that Ī”U = Ī”TĀ·(āˆ‚U/āˆ‚T)VĀ + Ī”VĀ·(āˆ‚U/āˆ‚V)TĀ expression, which we can now write as:

Ī”TĀ·(āˆ‚U/āˆ‚T)VĀ =Ā Ī”TĀ·(āˆ‚Q/āˆ‚T)VĀ = Ī”TĀ·CV

OK. So we’re done with the first term. Just to make sure we’re on the right track here, let’s have a quick look at the units here: the unit in which we should measureĀ CVĀ is, obviously, joule per degree (Kelvin), i.e. J/K. And then we multiply with Ī”T, which is measured in degrees Kelvin, and we get some amount in Joule. Fine. We’re done, indeed. šŸ™‚

Let’s look at the second term now, i.e. the Ī”VĀ·(āˆ‚U/āˆ‚V)TĀ term. Now, you may think that we couldĀ define CTĀ = (āˆ‚U/āˆ‚V)TĀ as the specific heat capacity at constant temperature because… Well… Hmm… It isĀ the amount of heat one must put into (or remove from) a substance in order to change its volume by one unit with the temperature held constant, isn’t it? So we writeĀ CTĀ =Ā (āˆ‚U/āˆ‚V)TĀ = (āˆ‚Q/āˆ‚V)TĀ and we’re done here too, aren’t we?

NO! HUGE MISTAKE!

It’s not that simple. Two very differentĀ things are happening here. Indeed, the change in (internal) energy Ī”U, as the volume changes byĀ Ī”VĀ while keeping the temperature constantĀ (we’re looking at that (āˆ‚U/āˆ‚V)TĀ factor here, and I’ll remind you of that subscript T a couple of times), consists of two parts:

  1. First, the volume is not being kept constant and, hence, the internal energy (U) changes because work is being done.
  2. Second, the internal energy (U) also changes because heat is being put in, so the temperature can be kept constant indeed.

So we cannot simplify. We’re stuck with the full thing: Ī”U = Ī”Q – PĪ”V, in which – PĪ”V is the (infinitesimal amount of) work that’s being done on the substance, and Ī”Q is the (infinitesimal amount of) heat that’s being put in. What can we do? How can we relate this to actual measurables?

Now, the logic is quite abstruse, so please be patient and bear with me. The key to the analysis is thatĀ diagram of the reversible Carnot cycle, with the shaded area representing the net work that’s being done, except that we’re now talkingĀ infinitesimallyĀ small changes in volume, temperature and pressure. So we redraw the diagram and get something like this:

Carnot 2Now, you can easily see the equivalence between the shaded area and the ΔPΔV rectangle below:

equivalenceSo the work done by the gas is the shaded area, whose surface is equal to Ī”PĪ”V. […] But… Hey, wait a minute!Ā You should object: we are not talking ideal engines here and, hence, we are notĀ going through a full Carnot cycle, are we? We’re calculating the change in internal energy when the temperature changes withĀ Ī”T, the volume changes withĀ Ī”V, and the pressure changes with Ī”P. Full stop. So we’re not going back to where we came from and, hence, we should not be analyzing this thing using the Carnot cycle, should we? Well… Yes and no. More yes than no. Remember we’re looking at the second term only here:Ā Ī”VĀ·(āˆ‚U/āˆ‚V)T. So we are changing the volume (and, hence, the internal energy) but the subscript in theĀ (āˆ‚U/āˆ‚V)TĀ term makes it clear we’re doing soĀ at constant temperature. In practice, that means we’re looking at a theoretical situation here that assumes a complete and fully reversible cycle indeed. Hence, the conceptual idea is, indeed, that we put some heat in, that the gas does some work as it expands, and that we then are actually putting some work back in to bring the gas back to its original temperature T. So, in short, yes, the reversible cycle idea applies.

[…]Ā I know, it’s veryĀ confusing. I am actually struggling with the analysis myself, so don’t be too hard on yourself. Think about it, but don’t lose sleep over it. šŸ™‚ I added a note on it in the P.S. to this post on it so you can check that out too. However, I need to get back to the analysis itself here. From our discussion of the Carnot cycle and ideal engines, we know that the work done is equal to the difference between the heat that’s being put in and the heat that’s being delivered:Ā W = Q1 – Q2. Now, because we’re talking reversible processes here, we also know that Q1/T1Ā = Q2/T2. Hence, Q2Ā = (TĀ 2/T1)Q1Ā and, therefore, the work done is also equal to W = Q1 – (TĀ 2/T1)Q1Ā =Ā Q1(1 – TĀ 2/T1) = Q1[(T1 – T2)/T1]= Q1(Ī”T/T1). Let’s now drop the subscripts by equating Q1Ā with Ī”Q, so we have:

W = ΔQ(ΔT/T)

You should noteĀ that Ī”Q is notĀ the difference between Q1Ā and Q2. It is not. Ī”Q is the heat we put in as it expands isothermally from volume V to volume V +Ā Ī”V. I am explicit about it because theĀ Ī” symbol usually denotes someĀ differenceĀ between two values. In case you wonder how we can do away with Q2, think about it. […] The answer is that we did notĀ really get away with it: the information is captured in the Ī”T factor, as T–ΔT is the final temperature reached by the gas as it expands adiabatically on the second leg of the cycle, and the change in temperature obviously depends on Q2! Again, it’s all quite confusing because we’re looking at infinitesimal changes only, but the analysis is valid. [Again, go through the P.S. of this post if you want more remarks on this, although I am not sure they’re going to help you much. The logic is really very deep.]

[…] OK… I know you’re getting tired, but we’re almost done. Hang in there.Ā So what do we have now? The work done by the gas as it goes through this infinitesimally small cycle is the shaded area in the diagram above, and it is equal to:

W = ΔPΔV = ΔQ(ΔT/T)

From this, it follows that Ī”Q = TĀ·Ī”VĀ·Ī”P/Ī”T. Now, you should look at the diagram once again to check what Ī”P actually stands for: it’s the change in pressure when the temperature changes at constant volume. Hence, using our partial derivative notation, we write:

Ī”P/Ī”T =Ā (āˆ‚P/āˆ‚T)V

We can now write Ī”Q = TĀ·Ī”VĀ·(āˆ‚P/āˆ‚T)VĀ and, therefore, we can re-writeĀ Ī”U = Ī”Q – PĪ”V as:

Ī”U = TĀ·Ī”VĀ·(āˆ‚P/āˆ‚T)V – PĪ”V

Now, dividing both sides by ΔV, and writing all using the partial derivative notation, we get:

Ī”U/Ī”V = (āˆ‚U/āˆ‚V)T = TĀ·(āˆ‚P/āˆ‚T)V – P

So now we know how to calculate the (āˆ‚U/āˆ‚V)TĀ factor, from measurable stuff, in that Ī”U = Ī”TĀ·(āˆ‚U/āˆ‚T)VĀ + Ī”VĀ·(āˆ‚U/āˆ‚V)TĀ expression, and so we’re done. Let’s write it all out:

Ī”U = Ī”TĀ·(āˆ‚U/āˆ‚T)VĀ + Ī”VĀ·(āˆ‚U/āˆ‚V)TĀ =Ā Ī”TĀ·CVĀ + Ī”VĀ·[TĀ·(āˆ‚P/āˆ‚T)V – P]

Phew! That was tough, wasn’t it? It was. Very tough. As far as I am concerned, this is probably the toughest of all I’ve written so far.

Dependent and independent variablesĀ 

Let’s pause to take stock of what we’ve done here. The expressions above should make it clear we’re actually treating temperature and volume as the independent variables, and pressure and energy as the dependent variables, or as functionsĀ of (other) variables, I should say. Let’s jot down the key equations once more:

  1. Ī”U = Ī”Q – PĪ”V
  2. Ī”U = Ī”TĀ·(āˆ‚U/āˆ‚T)VĀ + Ī”VĀ·(āˆ‚U/āˆ‚V)TĀ 
  3. (āˆ‚U/āˆ‚T)VĀ =Ā (āˆ‚Q/āˆ‚T)V = CV
  4. (āˆ‚U/āˆ‚V)T = TĀ·(āˆ‚P/āˆ‚T)V – P

It looks like Chinese, doesn’t it? šŸ™‚ What can we do with this? Plenty. Especially the first equation is really handy for analyzing and solving various practical problems. The second equation is much more difficult and, hence, less practical. But let’s try to apply this equation for actualĀ gases to an ideal gas—just to see if we’re getting our ideal gas law once again. šŸ™‚ We know that, for an ideal gas, the internal energy depends on temperature, notĀ on V. Indeed, if we change the volume but we keep the temperature constant, the internal energy should be the same, as it only depends on the motion of the molecules and their number. Hence,Ā (āˆ‚U/āˆ‚V)TĀ must equal zero and, hence, TĀ·(āˆ‚P/āˆ‚T)V – P = 0. Replacing the partial derivative with an ordinary one (not forgetting that the volume is kept constant), we get:

TĀ·(dP/dT) – P = 0 (constant volume)

⇔ (1/P)Ā·(dP/dT) = 1/T (constant volume)

Integrating both sides yields: lnP = lnT + constant. This, in turn, implies that P = T Ɨ constant. [Just re-write the first constant as the (natural) logarithm of some other constant, i.e. the second constant, obviously).] Now that’s consistent with our ideal gas P = NkT/V, because N, k and V are all constant. So, yes, the ideal gas law is a special case of our more general thermodynamical expression. Fortunately! šŸ™‚

That’s not very exciting, you’ll say—and you’re right. You may be interested – although I doubt it šŸ™‚Ā ā€“ in the chemists’ world view: they usually have performance data (read: values for derivatives) measured under constant pressure. The equations above then transform into:

  1. ΔH = Δ(U + P·V) = ΔQ + VΔP
  2. Ī”H = Ī”TĀ·(āˆ‚H/āˆ‚T)PĀ + Ī”PĀ·(āˆ‚H/āˆ‚P)TĀ 
  3. (āˆ‚H/āˆ‚P)T = –TĀ·(āˆ‚V/āˆ‚T)PĀ + V

H? Yes. H is another so-called state variable, so it’sĀ likeĀ entropy or internal energy but different. As they say in Asia: “Same-same but different.” šŸ™‚ It’sĀ definedĀ as H = U + PV and its name is enthalpy.Ā Why do we need it? Because some clever man noted that, if you take the total differential of PĀ·V, i.e.Ā Ī”(PĀ·V) = PĀ·Ī”V + VĀ·Ī”P, and our Ī”U = Ī”Q – PĀ·Ī”V expression, and you add both sides of both expressions, you getĀ Ī”(U + PĀ·V) = Ī”Q + VĪ”P. So we’ve substituted –P for V – so as to please the chemists – and all our equations hold provided we substitute U for H and, importantly, –P for V. [Note the sign switch is to be applied to derivatives as well: if we substitute P for –V, then āˆ‚P/āˆ‚T becomes āˆ‚(–V)/āˆ‚T = –(āˆ‚V/āˆ‚T)!

So that’s theĀ chemists’ model of the world, and they’ll usually measure the specific heat capacity at constant pressure, rather than at constant volume. Indeed, one can show the following:

(āˆ‚H/āˆ‚T)PĀ = (āˆ‚Q/āˆ‚T)PĀ =Ā CPĀ = the specific heat capacity at constant pressure

In short, while we referred to γ as the specific heat ratio in our previous posts, assuming we’re talking ideal gases only, we can now appreciate the fact there is actually no such thing asĀ theĀ specific heat: there are various variables and, hence, various definitions. Indeed, it’s not only pressure or volume: the specific heat capacity of some substance will usually also be expressed as a function of its mass (i.e. per kg), the number of particles involved (i.e. perĀ mole), or its volume (i.e. perĀ m3). In that case, we talk about the molar or volumetric heat capacity respectively. The name for the same thing expressed in joule per degree Kelvin and per kg (J/kgĀ·K) is the same: specific heat capacity. So we’ve got three different concepts here, and two ways of measuring them: at constant pressure or at constant volume. No wonder one gets quite confused when googlingĀ tables listing the actual values! šŸ™‚

Now, there’s one question left: why is γ being referred to as the specific heat ratio? The answer is simple: it actually is the ratio of the specific heat capacities CPĀ andĀ CV. Hence, γ is equal to:

γ = CP/CV

I could show you how that works. However, I would just be copying the Wikipedia article on it, so I won’t do that: you’re sufficiently knowledgeable now to check it out yourself, and verify it’s actually true. Good luck with it ! In the process, please also do check why CPĀ is always larger than CVĀ so you can explain why γ is always larger than one. šŸ™‚

Post scriptum: As usual, Feynman’s Lectures, were the inspiration here—once more. Now, Feynman has a habit of ‘integrating’ expressions and, frankly, I never found a satisfactory answer to a pretty elementary question: integration in regard to what variable? His exposĆ© on both the ideal as well as the actual gas law has enlightened me. The answer is simple: it doesn’t matter. šŸ™‚ Let me show that by analyzing the following argument of Feynman:

expose

So… What is that ‘integration’ that ‘yields’ that γlnV + lnP = lnC expression? Are we solving some differential equation here? Well… Yes. But let’s be practical and take the derivative of the expression in regard to V, P and T respectively. Let’s first see where we come from. The fundamental equation is PV = (γ–1)U. That means we’ve got two ‘independent’ variables, and one that ‘depends’ on the others: if we fix P and V, we have U, or if we fix U, then P and V are in an inversely proportional relationship. That’s easy enough. We’ve got three ‘variables’ here: U, P and V—or, in differential form, dU, dP and dV. However, Feynman eliminates one by noting that dU = –PdV. He rightly notes we can only do that because we’re talking adiabatic expansion/compression here:Ā all the work done while expanding/compressing the gas goes into changing the internal energy: no heat is added or removed. Hence, there is no dQ term here.

So we are left with two ‘variables’ only now: P and V, or dP and dV when talking differentials. So we can choose: P depends on V, or V depends on P. If we think of V as the independent variable, we can write:

d[γ·lnV + lnP]/dV = γ·(1/V)·(dV/dV) + (1/P)·(dP/dV), while d[lnC]/dV = 0

So we have γ·(1/V)·(dV/dV) + (1/P)·(dP/dV) = 0, and we can then multiply sides by dV to get:

(γ·dV/V) + (dP/P) = 0,

which is the coreĀ equation in this argument, so that’s the one we started off with. Picking P as the ‘independent’ variable and, hence, integrating with respect to P yields the same:

d[γ·lnV + lnP]/dP = γ·(1/V)·(dV/dP) + (1/P)·(dP/dP), while d[lnC]/dP = 0

Multiplying both sides by dP yields the same thing: (γ·dV/V) + (dP/P) = 0. So it doesn’t matter, indeed. But let’s be smart and assume both P and V, or dP and dV, depend on some implicitĀ variable—a parameterĀ really. The obvious candidate is temperatureĀ (T). So we’ll now integrate and differentiate in regard to T. We get:

d[γ·lnV + lnP]/dT = γ·(1/V)·(dV/dT) + (1/P)·(dP/dT), while d[lnC]/dT = 0

We can, once again, multiply both sides with dT and – surprise, surprise! – we get the same result:Ā 

(γ·dV/V) + (dP/P) = 0

The point is that the γlnV + lnP = lnC expression isĀ damnĀ valid, and C or lnC or whatever is ‘the constant of integration’ indeed, in regard to whatever variable: it doesn’t matter. So then we can, indeed, take the exponential of both sides (which is much more straightforward than ‘integrating both sides’), so we get:

eγlnV + lnP = elnC = C

It then doesn’t take too much intelligence to see that eγlnV + lnP = e(lnV)γ+lnPĀ = e(lnV)γ·elnPĀ =Ā Vγ·P = PĀ·Vγ. So we’ve got the grand result that what we wanted:Ā PVγ = C, with C some constant determined by the situation we’re in (think of the size of the box, or the density of the gas).

So, yes, we’ve got a ‘law’ here. We should just remind ourselves,Ā always, that it’s only valid when we’re talking adiabatic compression or expansion: so weĀ we do not add or remove heat energyĀ or, as Feynman puts it, much more succinctly, “no heat is being lost“. And, of course, we’re also talking ideal gases only—which excludes a number of realĀ substances. šŸ™‚ In addition, we’re talking adiabatic processes only: we’re not adding nor removing heat.

It’s a weird formula: the pressure times the volume to the 5/3 power is a constant for monatomic gas. But it works: as long as individual atoms are not bound to each other, the law holds. As mentioned above, when variousĀ molecularĀ states, with associated energy levels are at play, it becomes an entirely different ballgame. šŸ™‚

I should add one final note as to the functional form ofĀ PVγ = C. We can re-write it as P = C/Vγ. Because The shape of that graph is similar to the P = NkT/V relationship we started off with. Putting the two equations side by side, makes it clear our constant and temperature are obviously related one to another, but they are not directly proportional to each other. In fact, as the graphs below clearly show, the P = NkT/V gives us these isothermal lines on the pressure-volume graph (i.e. they show P and V are related at constant temperature), while the P = C/Vγ equation gives us the adiabatic lines. Just google an online function graph tool, and you can now draw your own diagrams of the Carnot cycle! Just change the denominator (i.e. the constants C and T in both equations). šŸ™‚

graphNow, I promised I would say something more about that infinitesimal Carnot cycle: why is it there? Why don’t we limit the analysis to just the first two steps? In fact, the shortest and best explanation I can give is something like this: think of the whole cycle as the first step in a reversible process really. We put some heat in (Ī”Q) and the gas does some work, but so that heat has to go through the whole body of gas, and the energy has to go somewhere too. In short, the heat and the work is not being absorbed by the surroundings but it all stays in the ‘system’ that we’re analyzing, so to speak, and that’s why we’re going through the full cycle, not the first two steps only. Now, this ‘answer’ may or may not satisfy you, but I can’t do better. You may want to check Feynman’s explanation itself, but he’s very short on this and, hence, I think it won’t help you much either. 😦

Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 16, 2020 as a result of a DMCA takedown notice from The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/
Some content on this page was disabled on June 17, 2020 as a result of a DMCA takedown notice from Michael A. Gottlieb, Rudolf Pfeiffer, and The California Institute of Technology. You can learn more about the DMCA here:

https://wordpress.com/support/copyright-and-the-dmca/

The Strange Theory of Light and Matter (III)

Pre-script (dated 26 June 2020): This post has become less relevant (even irrelevant, perhaps) because my views on all things quantum-mechanical have evolved significantly as a result of my progression towards a more complete realist (classical) interpretation of quantum physics. I keep blog posts like these mainly because I want to keep track of where I came from. I might review them one day, but I currently don’t have the time or energy for it. šŸ™‚

Original post:

This is my third and final comments on Feynman’s popular little booklet: TheĀ Strange Theory of Light and Matter, also known as Feynman’sĀ Lectures on Quantum ElectrodynamicsĀ (QED).

TheĀ origin of this short lecture series is quite moving: the death of Alix G. Mautner, a good friend of Feynman’s. She was always curious about physics but her career was in English literature and so she did not manage the math. Hence, Feynman introduces this 1985 publication by writing: “Here are the lectures I really prepared for Alix, but unfortunately I can’t tell them to her directly, now.”

Alix Mautner died from a brain tumor, and it is her husband, Leonard Mautner, who sponsored the QED lectures series at the UCLA, which Ralph Leigton transcribed and published as the booklet that we’re talking about here. Feynman himself died a few years later, at the relatively young age of 69. Tragic coincidence: he died of cancer too. Despite all this weirdness, Feynman’s QED never quite got the sameĀ iconicĀ status of, let’s say, Stephen Hawking’sĀ Brief History of Time.Ā I wonder why, but the answer to that question is probably in the realm of chaos theory. šŸ™‚ I actually just saw the movie on Stephen Hawking’s life (The Theory of Everything), and I noted another strange coincidence: Jane Wilde, Hawking’s first wife,Ā also has a PhD in literature. It strikes me that, while the movie documents that Jane Wilde gave Hawking three children, after which he divorced her to marry his nurse, Elaine, the movie does not mention that he separated from Elaine too, and that he has some kind of ‘working relationship’ with Jane again.

Hmm… What to say? I should get back to quantum mechanics here or, to be precise, to quantum electrodynamics.

One reason why Feynman’s Strange Theory of Light and MatterĀ did not sell like Hawking’s BriefĀ History of Time, might wellĀ be that, in some places, the text is not entirely accurate. Why?Ā Who knows? It would make for an interesting PhD thesis in History of Science. Unfortunately,Ā I have no time for such PhD thesis. Hence, I must assume that Richard Feynman simply didn’t have much time or energy left to correct some of the writing ofĀ Ralph Leighton, who transcribed and edited these four short lectures a few years before Feynman’s death.Ā Indeed, when everything is said and done, Ralph Leighton is not a physicist and, hence, I think he did compromise – just a little bit – on accuracy for the sake of readability. Ralph Leighton’s father, Robert Leighton,Ā an eminent physicist who worked with Feynman, would probably have done a much better job.

I feel that one should notĀ compromise on accuracy, even when trying to write something reader-friendly. That’s why I am writing this blog, and why I am writing three posts specifically on this little booklet. Indeed, while I’d warmly recommend that little book on QED as an excellent non-mathematical introduction to the weird world of quantum mechanics, I’d also say that, while Ralph Leighton’s story is great, it’s also, in some places, not entirelyĀ accurate indeed.

So… Well… I want to do better than Ralph Leighton here. Nothing more. Nothing less. šŸ™‚ Let’s go for it.

I. Probability amplitudes: whatĀ areĀ they?

The greatest achievement of that little QED publication is that it manages to avoid any reference to wave functions and other complicated mathematical constructs: all of the complexity of quantum mechanics is reduced toĀ three basic eventsĀ or actions and, hence, three basic amplitudesĀ which are represented as ‘arrows’—literally.

Now… Well… You may or may not know thatĀ a (probability)Ā amplitude is actually aĀ complex number, but it’s not so easy to intuitively understand the concept of a complex number. In contrast, everyone easily ‘gets’ the concept of an ‘arrow’. Hence, from a pedagogical point of view, representing complex numbers by some ‘arrow’ is truly a stroke of genius.

Whatever we call it, a complex number or an ‘arrow’, a probability amplitude is something with (a) a magnitudeĀ and (b) a phase. As such, it resembles a vector, but it’s not quite the same, if only because we’ll impose some restrictions on the magnitude. But I shouldn’t get ahead of myself. Let’s start with the basics.

A magnitude is some real positiveĀ number, like a length, but you shouldĀ not associate it with some spatial dimension in physical space: it’s just a number. As for the phase, weĀ could associate that concept with some directionĀ but, again, you should just think of it as a direction in aĀ mathematicalĀ space,Ā not in the realĀ (physical)Ā space.

Let me insert a parenthesis here. If I say the ‘real’ or ‘physical’ space, I mean the space in which the electrons and photons and all other real-life objects that we’re looking at exist and move. That’s a non-mathematical definition. In fact, in math, the real space is defined as a coordinate space, with sets of real numbers (vectors) as coordinates, so… Well… That’s a mathematical space only, not the ‘real’ (physical) space. So the real (vector) space is not real. šŸ™‚ The mathematical real space may, or may not, accuratelyĀ describeĀ the real (physical) space. Indeed, you may have heard that physical space is curved because of the presence of massive objects, which means that the real coordinate space will actuallyĀ notĀ describe it very accurately. I know that’s a bit confusing but I hope you understand what I mean: if mathematicians talk about the real space, they do not mean the real space. They refer to a vector space, i.e. a mathematical construct. To avoid confusion, I’ll use the term ‘physical space’ rather than ‘real’ space in the future. So I’ll let the mathematicians get away with using the term ‘real space’ for something that isn’t real actually. šŸ™‚

End of digression. Let’s discuss these two mathematical concepts – magnitude and phase – somewhat more in detail.

A.Ā The magnitude

Let’s start with the magnitude or ‘length’ of our arrow. We know that we have to squareĀ these lengths to find some probability, i.e. some real number betweenĀ 0 and 1. Hence, the length of our arrows cannot be larger than one. That’s the restriction I mentioned already, and this ‘normalization’ condition reinforces the point that these ‘arrows’ do not have any spatial dimension (not in any realĀ space anyway): they represent aĀ function. To be specific, they represent a wavefunction.

If we’d be talking complex numbers instead of ‘arrows’, we’d say the absolute valueĀ of the complex number cannot be larger than one. We’d also say that, to find the probability, we should take theĀ absoluteĀ square of the complex number, so that’s theĀ square of theĀ magnitudeĀ orĀ absoluteĀ value of the complex number indeed. We cannot just square the complex number: it has to be the square of the absolute value.

Why? Well… Just write it out. [You can skip this section if you’re not interested in complex numbers, but I would recommend you try to understand. It’s not that difficult. Indeed, if you’re reading this, you’re most likely to understand somethingĀ of complex numbers and, hence, you should be able to work your way through it. Just remember that a complex number is like a two-dimensional number, which is why it’s sometimes written using bold-face (z), rather than regular font (z). However, I should immediately add this convention is usually notĀ followed. I like the boldface though, and so I’ll try to use it in this post.] The square of a complex number z = a + bi is equal to z2Ā = a2Ā + 2abi – b2, while the square of its absolute value (i.e. the absolute square) is |z|2Ā = [√(a2Ā + b2)]2Ā = a2Ā + b2. So you can immediately see that the square and the absolute square of a complex numbers are two very different things indeed: it’s not only the 2abiĀ term, but there’s also the minus sign in the first expression, because of theĀ i2Ā = –1 factor. In case of doubt, always remember that the square of a complex number may actually yield aĀ negativeĀ number, as evidenced by the definition of the imaginary unit itself:Ā i2Ā = –1.

End of digression. Feynman and Leighton manage to avoid any reference to complex numbers in that short series of four lectures and, hence, all they need to do is explain how one squares a length. Kids learn how to do that when making a square out of rectangular paper: they’ll fold one corner of the paper until it meets the opposite edge, forming a triangle first. They’ll then cut or tear off the extra paper, and then unfold. Done. [I could note that the folding is a 90 degree rotation of the original length (or width, I should say) which, in mathematical terms, is equivalent to multiplying that length with the imaginary unit (i). But I am sure the kids involved would think I am crazy if I’d say this. šŸ™‚ So let me get back to Feynman’s arrows.

B. The phase

Feynman and Leighton’s second pedagogical stroke of genius is the metaphor of theĀ ‘stopwatch’ and the ‘stopwatch hand’ for the variableĀ phase. Indeed, although I think it’s worth explaining why zĀ = a + bi = rcosφ + irsinφ in the illustration below can be written as z =Ā reiφ = |z|eiφ, understanding Euler’s representation ofĀ complex number as a complex exponential requires swallowing a very substantial piece ofĀ math and, if you’d want to do that, I’ll refer you to one of my posts on complex numbers).

Complex_number_illustration

The metaphor of the stopwatch represents a periodic function. To be precise, it represents a sinusoid, i.e. a smooth repetitive oscillation. Now, the stopwatchĀ handĀ represents the phase of that function, i.e. the φ angle in the illustration above. That angle isĀ a function of time: the speed with which the stopwatch turns is related to some frequency, i.e. the number of oscillations per unit of time (i.e. per second).

You should now wonder: what frequency? What oscillations are we talking about here? Well… As we’re talking photons and electrons here, we should distinguish the two:

  1. For photons, the frequency is given by Planck’s energy-frequency relation, which relates the energy (E) of a photon (1.5 to 3.5 eV for visible light) to its frequency (ν). It’s a simple proportional relation, with Planck’s constant (h) as the proportionality constant: E = hν, or ν = E/h.
  2. For electrons, we have the de BroglieĀ relation, which looks similar to the Planck relation (E = hf, or f = E/h) but, as you know, it’s something different. Indeed, these so-calledĀ matter wavesĀ are not so easy to interpret because there actually is no precise frequency f. In fact, the matter wave representing some particle in space will consist of a potentially infinite number of waves, all superimposed one over another, as illustrated below.

Sequential_superposition_of_plane_waves

For the sake of accuracy, I should mention that the animation above has its limitations: the wavetrain is complex-valued and, hence, has a real as well as an imaginary part, so it’s something like the blob underneath. Two functions in one, so to speak: the imaginary part follows the real part with a phase difference of 90 degrees (or Ļ€/2 radians). Indeed, if the wavefunction is a regular complex exponential reiĪø, then rsin(φ–π/2) = rcos(φ), which proves the point: we have two functions in one here. šŸ™‚ I am actually just repeating what I said before already: the probability amplitude, or the wavefunction, is a complex number. You’ll usually see it written asĀ ĪØ (psi) or Φ (phi). Here also, using boldface (ĪØĀ or Φ instead ofĀ ĪØ or Φ) would usefully remind the reader that we’re talking something ‘two-dimensional’ (in mathematical space, that is), but this convention is usuallyĀ notĀ followed.

Photon wave

In any case… Back to frequencies. The point to note is that, when it comes to analyzing electrons (or any other matter-particle), we’re dealing with a range of frequencies f really (or, what amounts to the same, a range of wavelengthsĀ Ī») and, hence, we should writeĀ Ī”f =Ā Ī”E/h, which is just one of the many expressions of the Uncertainty Principle in quantum mechanics.

Now, that’s just one of the complications. Another difficulty is that matter-particles, such as electrons, have some rest mass, and so that enters the energy equation as well (literally). Last but not least, one should distinguish between the group velocity and the phase velocity of matter waves. As you can imagine, that makes for a veryĀ complicated relationship between ‘the’ wavelength and ‘the’ frequency. In fact, what I write above should make it abundantly clear that there’s no such thing as the wavelength, or the frequency: it’s a range really, related to the fundamental uncertainty in quantum physics. I’ll come back to that, and so you shouldn’t worry about it here. Just note that the stopwatch metaphor doesn’t work very well for an electron!

In his postmortemĀ lectures for Alix Mautner, Feynman avoids all these complications. Frankly, I think that’s a missed opportunity because I doĀ notĀ think it’s all that incomprehensible. In fact, I write all that follows because I do want you to understand the basics of waves.Ā It’s not difficult.Ā High-school math is enough here. Let’s go for it.

One turn of the stopwatch corresponds to one cycle. One cycle, or 1 Hz (i.e. one oscillation per second) covers 360 degrees or, to use a more natural unit, 2Ļ€ radians. [Why is radian a more natural unit? Because it measures an angle in terms of the distance unit itself, rather than in arbitrary 1/360 cuts of a full circle. Indeed, remember that the circumference of the unit circle is 2Ļ€.] So our frequency ν (expressed in cycles per second) corresponds to a so-called angular frequency ω = 2πν. From this formula, it should be obvious that ω is measured in radians per second.

We can also link this formula to the periodĀ of the oscillation, T,Ā i.e. the duration of one cycle. T = 1/ν and, hence, ω = 2Ļ€/T. It’s all nicely illustrated below. [And, yes, it’s an animation from Wikipedia: nice and simple.]

AngularFrequency

The easy math above now allows us to formally write the phase of a wavefunction – let’s denote the wavefunction as φ (phi), and the phase as Īø (theta) – as a function of time (t) using the angular frequency ω. So we can write: ĪøĀ = ωt = 2π·ν·t. Now, the wave travels through space, and the two illustrations above (i.e. the one with the super-imposed waves, and the one with the complex wave train) would usually represent a waveĀ shapeĀ at some fixed point in time. Hence, the horizontal axis is not t but x. Hence, we can and should write the phase not only as a function of time but also of space. So how do we do that? Well… If the hypothesis is that the wave travels through space at someĀ fixedĀ speedĀ c, then its frequency ν will also determine its wavelengthĀ Ī». It’s a simple relationship: cĀ = λν (the number of oscillations per secondĀ times the length of one wavelength should give you the distance traveled per second, so that’s, effectively, the wave’s speed).

Now that we’ve expressed the frequency inĀ radiansĀ per second, we can also express the wavelength inĀ radiansĀ per unit distance too. That’s what the wavenumber does: think of it as the spatial frequency of the wave. We denote the wavenumber by k, and write: k = 2Ļ€/Ī». [Just do a numerical example when you have difficulty following. For example, if you’d assume the wavelength is 5 units distance (i.e. 5Ā meter) – that’s a typical VHF radio frequency: ν = (3Ɨ108Ā m/s)/(5 m) = 0.6Ɨ108 Hz = 60 MHz – then that would correspond to (2Ļ€ radians)/(5 m) ā‰ˆ 1.2566 radiansĀ per meter. Of course, we can also express the wave number inĀ oscillationsĀ per unit distance. In that case, we’d have to divide k by 2Ļ€, because one cycle corresponds to 2Ļ€ radians. So we get the reciprocal of the wavelength: 1/Ī». In our example, 1/Ī» is, of course, 1/5 = 0.2, so that’s a fifth of a full cycle. You can also think of it as the number of waves (or wavelengths) per meter: if the wavelength is Ī», then one can fit 1/Ī» waves in a meter.

waveform-showing-wavelength

Now, from the ω = 2πν, cĀ = λν and k = 2Ļ€/Ī» relations, it’s obvious that k = 2Ļ€/Ī» = 2Ļ€/(c/ν) = (2πν)/c = ω/c. To sum it all up, frequencies and wavelengths, in time and in space, are all related through the speed of propagation of the wave c. More specifically, they’re related as follows:

c = λν = ω/k

From that, it’s easy to see that k = ω/c, which we’ll use in a moment. Now, it’s obvious that the periodicity of the wave implies that we can find the same phase by going one oscillation (or a multiple number of oscillations back or forward in time, or in space. In fact, we can also find the same phase by letting both time and space vary. However, if we want to do that, it should be obvious that we should either (a) go forward in space and back in time or, alternatively, (b) go back in space and forward in time. In other words, if we want to get the same phase, then time and space sort of substitute for each other. Let me quote Feynman on this: “This is easily seen by considering the mathematical behavior of a(tāˆ’r/c). Evidently, if we add a little timeĀ Ī”t, we get the same value for a(tāˆ’r/c) as we would have if we had subtracted a little distance: Ī”rĀ =Ā āˆ’cĪ”t.” The variable a stands for the acceleration of an electric charge here, causing an electromagnetic wave, but the same logic is valid for the phase, with a minor twist though: we’re talking a nice periodic function here, and so we need to put the angular frequency in front. Hence, the rate of change of the phase in respect to time is measured by the angular frequency ω. In short, we write:

Īø = ω(t–x/c) = ωt–kx

Hence, we can re-write the wavefunction, in terms of its phase, as follows:

φ(Īø) = φ[Īø(x, t)] = φ[ωt–kx]

Note that, if the wave would be traveling in the ‘other’ direction (i.e. in the negativeĀ x-direction), we’d write φ(Īø) = φ[kx+ωt]. Time travels in one direction only, of course, but so one minus sign has to be there because of the logic involved in adding time and subtracting distance. You can work out an example (with a sine or cosine wave, for example) for yourself.

So what, you’ll say? Well… Nothing. I just hope you agree that all of this isn’t rocket science: it’s just high-school math. But so it shows you what that stopwatch really is and, hence, I – but who am I? – would have put at least one or two footnotes on this in a text like Feynman’s QED.

Now, let me make a much longer and more serious digression:

Digression 1: on relativity and spacetime

As you can see from the argument (or phase) of that wave function φ(Īø) = φ[Īø(x, t)] = φ[ωt–kx] = φ[–k(x–ct)], any wave equation establishes a deep relation between the wave itself (i.e. the ‘thing’ we’re describing) and space and time. In fact, that’s what the whole wave equation is all about! So let me say a few things more about that.

Because you know a thing or two about physics, you may ask: when we’re talking time,Ā whose timeĀ are we talking about?Ā Indeed, if we’re talking photons going from A to B, these photons will be traveling at or near the speed of light and, hence, their clock, as seen from our (inertial) frame of reference, doesn’t move. Likewise, according to the photon,Ā ourĀ clock seems to be standing still.

Let me put the issue to bed immediately: we’re looking at things from our point of view. Hence, we’re obviously using ourĀ clock, not theirs. Having said that,Ā the analysis is actually fully consistent with relativity theory. Why? Well… What do you expect? If it wasn’t, the analysis would obviously notĀ be valid. šŸ™‚ To illustrate that it’s consistent with relativity theory, I can mention, for example, that the (probability) amplitude for a photon to travel from point A to B depends on the spacetime interval, which is invariant. Hence, A and B are four-dimensional points inĀ spacetime, involving both spatial as well as time coordinates: A = (xA, yA, zA, tA) and BĀ = (xB, yB, zB, tB). And so the ‘distance’ – as measured through the spacetime interval – is invariant.

Now, having said that, we should draw some attention to the intimate relationship between space and time which, let me remind you, results from the absoluteness of the speed of light. Indeed, one will always measure the speed of lightĀ cĀ as being equal to 299,792,458 m/s,Ā always and everywhere.Ā It doesĀ notĀ depend on your reference frame (inertial or moving). That’s why the constant c anchors all laws in physics, and why we can write what we write above, i.e. include both distance (x) as well as time (t) in the wave function φ = φ(x, t) = φ[ωt–kx] = φ[–k(x–ct)]. The k and ω are related through the ω/k =Ā c relationship:Ā the speed of light links the frequency in time (ν = ω/2π = 1/T) with the frequency in space (i.e. the wavenumber or spatial frequencyĀ k).Ā There is only degree of freedom here: the frequency—in space or in time, it doesn’t matter: ν and ω are notĀ independent. Ā [As noted above, the relationship between the frequency in time and in space isĀ notĀ so obvious for electrons, or for matter waves in general: for those matter-waves, we need to distinguish group and phase velocity, and so we don’t have a unique frequency.]

Let me make another small digression within the digression here. Thinking about travel at the speed of light invariably leads to paradoxes. In previous posts, I explained the mechanism of light emission: a photon is emitted – one photon only – when an electron jumps back to its ground state after being excited. Hence, we may imagine a photon as a transient electromagnetic wave–something like what’s pictured below. Now, the decay time of this transient oscillation (Ļ„) is measured inĀ nanoseconds, i.e. billionths of a second (1 ns = 1Ɨ10–9Ā s): the decay time for sodium light, for example, is some 30 ns only.

decay time

However, because of the tremendous speed of light, that still makes for a wavetrainĀ that’s like ten meter long,Ā at least (30Ɨ10–9Ā s timesĀ 3Ɨ108Ā m/s is nine meter, but you should note that the decay time measures the time for the oscillation to die out by a factor 1/e, so the oscillation itself lasts longer than that). Those nine or ten meters cover like 16 to 17 million oscillations (the wavelength of sodium light is aboutĀ 600 nm and, hence, 10 meter fits almost 17 million oscillations indeed). Now, how can we reconcile the image of a photon as a ten-meter long wavetrain with the image of a photon as a pointĀ particle?

The answer to that question is paradoxical: from ourĀ perspective,Ā anything traveling at the speed of light – including this nine or ten meter ‘long’ photon – will have zero length because of the relativistic length contraction effect. Length contraction? Yes. I’ll let you look it up, because… Well… It’s not easy to grasp. Indeed, from the three measurable effects on objects moving at relativistic speeds – i.e. (1) an increase of the mass (the energy needed to further accelerate particles in particle accelerators increases dramatically at speeds nearer to c), (2) time dilation, i.e. a slowing down of the (internal) clock (because of their relativistic speeds when entering the Earth’s atmosphere, the measured half-life of muons is fiveĀ times that when at rest), and (3) length contraction – length contraction is probably the most paradoxical of all.

Let me end this digression with yet another short note. I said that one will always measure the speed of lightĀ cĀ as being equal to 299,792,458 m/s,Ā always and everywhereĀ and, hence, that it doesĀ notĀ depend on your reference frame (inertial or moving). Well… That’s true and not true at the same time. I actually need to nuance that statement a bit in light of what follows: anĀ individualĀ photon does have an amplitude to travel faster or slower than c, and when discussing matter waves (such as the wavefunction that’s associated with an electron), we can have phase velocities that are faster than light! However, when calculating those amplitudes, cĀ is a constant.

That doesn’t make sense, you’ll say. Well… What can I say? That’s how it is unfortunately. I need to move on and, hence, I’ll end this digression and get back to the main story line. Part I explained what probability amplitudes are—or at least tried to do so. Now it’s time for part II: the building blocks of all of quantum electrodynamics (QED).

II. The building blocks: P(A to B), E(A to B) and j

The three basic ‘events’ (and, hence, amplitudes) in QED are the following:

1. P(A to B)

P(A to B) is the (probability) amplitude for a photon to travel from point A to B. However, I should immediately note that A and B are points in spacetime. Therefore, we associate them not only with some specific (x, y, z) position in space, but also with a some specificĀ time t.Ā Now, quantum-mechanical theory gives us an easy formula for P(A to B): it depends on the so-called (spacetime) interval between the two points A and B, i.e. IĀ =Ā Ī”r2 – Δt2Ā = (x2–x1)2+(y2–y1)2+(z2–z1)2 – (t2–t1)2. The point to note is that the spacetime interval takes both the distance in space as well as the ā€˜distance’ in time into account. As I mentioned already, this spacetime interval does not depend on our reference frame and, hence, it’s invariant (as long as we’re talking reference frames that move with constant speed relative to each other). Also note that we should measure time and distance in equivalent units when using that Ī”r2 – Δt2Ā formula for I. So we either measure distance in light-seconds or, else, we measure time in units that correspond to the time that’s needed for light to travel one meter. If no equivalent units are adopted, the formula isĀ I =Ā Ī”r2 – cĀ·Ī”t2.

Now, in quantum theory, anything is possible and, hence, not only do we allow for crooked paths, but we also allow for the difference in time to differ from Ā the time you’d expect a photon to need to travel along some curve (whose length we’ll denote by l), i.e. l/c. Hence, our photon may actually travel slower or faster than the speed of light c! There is one lucky break, however, that makes all come out alright: it’s easy to show that the amplitudes associated withĀ the odd paths and strange timings generallyĀ cancel each other out. [That’s what the QED booklet shows.] Hence, what remains, are the paths that are equal or, importantly, those thatĀ very near to the so-called ‘light-like’ intervals in spacetime only. TheĀ netĀ result is that light – even one single photon – effectively uses a (very) small core of space as it travels, as evidenced by the fact thatĀ even one single photon interferesĀ with itselfĀ when traveling through a slit or a small hole!

[If you now wonder what it means for a photon to interfere for itself, let me just give you the easy explanation: it may change its path. We assume it was traveling in a straight line – if only because it left the source at some point in time and then arrived at the slit obviously – but so it no longer travels in a straight line after going through the slit. So that’s what we mean here.]

2.Ā E(A to B)

E(A to B) is the (probability) amplitude for an electron to travel from point A to B. The formula for E(A to B) is much more complicated, and it’s the one I want to discuss somewhat more in detail in this post. It depends on some complex numberĀ jĀ (see the next remark) and some real number n.

3. j

Finally, an electron could emit or absorb a photon, and the amplitude associated with this event is denoted byĀ j, for junction number. It’s the same number j as the one mentioned when discussing E(A to B) above.

Now, this junction number is often referred to as the coupling constant or the fine-structure constant. However, the truth is, as I pointed out in my previous post, that these numbers are related, but they are not quite the same: α is the squareĀ of j, so we have α = j2. There is also one more, related, number: the gauge parameter, which is denoted by g (despite the g notation, it has nothing to do with gravitation). The value of g is the square root of 4πε0α, so g2Ā = 4πε0α. I’ll come back to this. Let me first make an awfully long digression on the fine-structure constant. It will be awfully long. So long that it’s actually part of the ‘core’ of this post actually.

Digression 2: on the fine-structure constant, Planck units and the Bohr radius

The value forĀ jĀ is approximately –0.08542454.

How do we know that?

The easy answer to that question is: physicists measured it. In fact, they usually publish the measured value as the square root of the (absolute value) of j, which is that fine-structure constant α. Its value is published (and updated) by the US National Institute on Standards and Technology. To be precise, the currently accepted value of α is 7.29735257Ɨ10āˆ’3. In case you doubt, just check that square root:

jĀ = –0.08542454 ā‰ˆ ā€“āˆš0.00729735257 =Ā ā€“āˆšĪ±

As noted in Feynman’s (or Leighton’s) QED, older and/or more popular books will usually mention 1/α as the ‘magical’ number, so the ‘special’ number you may have seen is the inverse fine-structure constant, which is about 137, but not quite:

1/α = 137.035999074 ± 0.000000044

I am adding the standard uncertainty just to give you an idea of how precise these measurements are. šŸ™‚ About 0.32 parts per billion (just divide the 137.035999074 number by the uncertainty). So that‘s the number that excites popular writers, including Leighton. Indeed, as Leighton puts it:

“Where does this number come from?Ā Nobody knows. It’s one of the greatest damn mysteries of physics: a magic number that comes to us with no understanding by man. You might say the “hand of God” wrote that number, and “we don’t know how He pushed his pencil.” We know what kind of a dance to do experimentally to measure this number very accurately, but we don’t know what kind of dance to do on the computer to make this number come out, without putting it in secretly!”

Is it Leighton, or did Feynman really say this? Not sure. WhileĀ theĀ fine-structure constant is a very special number, it’s not the only ‘special’ number. In fact, we derive it from other ‘magical’ numbers. To be specific, I’ll show you how we derive it from the fundamental propertiesĀ – as measured, of course – of the electron. So, in fact, I should say that weĀ doĀ know how to make this number come out, which makes me doubt whether Feynman really said what Leighton said he said. šŸ™‚

So we canĀ derive α from some other numbers. That brings me to theĀ more complicated answer to the question as to what the value of jĀ really is: j‘s value isĀ theĀ electron chargeĀ expressed in Planck units, which I’ll denote by –eP:

j = –eP

[You may want to reflect on this, and quickly verify on the Web. The Planck unit of electric charge, expressed inĀ Coulomb, is about 1.87555Ɨ10–18Ā C. If you multiply that j = –eP, so with –0.08542454, you get the right answer: the electron charge is about –0.160217Ɨ10–18Ā C.]

Now thatĀ is strange.

Why? Well… For starters, when doing all those quantum-mechanical calculations, we like to think of j as a dimensionless number: a coupling constant. But so here we do have a dimension: electric charge.

Let’s look at the basics. IfĀ jĀ is ā€“āˆšĪ±, and it’s also equal to –eP, then the fine-structure constant must also be equal to the square of the electron charge eP, so we can write:

α = eP2

You’ll say: yes, so what?Ā Well… I am pretty sure that, if you’ve ever seen a formula for α, it’s surely notĀ this simple j = –ePĀ or α =Ā eP2Ā formula. What you’ve seen, most likely, is one or more of the following expressions below :

Fine-structure constant formula

That’s a pretty impressive collection of physical constants, isn’t it? šŸ™‚ They’re all different but, somehow, when we combine them in one or the other ratio (we have not less than fiveĀ different expressions here (each identity is a separate expression), and I could give you a few more!), we get the very same number: α.Ā Now thatĀ is what I call strange.Ā TrulyĀ strange. Incomprehensibly weird!

You’ll say… Well… Those constants must all be related…Ā Of course!Ā That’s exactly the point I am making here. They are, but look how different they are: meĀ measures mass, reĀ measures distance, eĀ is a charge, and so these are all very different numbers with very different dimensions. Yet, somehow, they are all related through this α number. Frankly, I do not know of any other expression that better illustrates some kind of underlying unity in Nature than the one with those five identities above.

Let’s have a closer look at those constants. You know most of them already. The only constants you may not haveĀ seen before are μ0,Ā RKĀ and, perhaps, reĀ as well asĀ meĀ . However, these can easily be defined as some easy function of the constants that you didĀ seeĀ before, so let me quickly do that:

  1. The μ0Ā constant is the so-called magnetic constant. It’s something similar as ε0Ā and it’s referred to as the magneticĀ permeability of the vacuum. So it’s just like the (electric)Ā permittivity of the vacuum (i.e. the electric constant ε0) and the only reason why this blog hasn’t mentioned this constant before is because I haven’t really discussed magnetic fields so far. I only talked about the electric field vector. In any case, you know that the electric and magnetic force are part and parcel of the same phenomenon (i.e. theĀ electromagneticĀ interaction between charged particles) and, hence, they are closely related. To be precise, μ0ε0Ā = 1/c2Ā = c–2.Ā So that shows the first and second expression for α are, effectively, fully equivalent.Ā [Just in case you’d doubt that μ0ε0Ā = 1/c2, let me give you the values: μ0Ā = 4π·10–7 N/A2, and ε0Ā = (1/4π·c2)Ā·107Ā C2/NĀ·m2. Just plug them in, and you’ll see it’s bang on. Moreover, note that the ampereĀ (A) unit is equal to the coulomb per second unit (C/s), so even the units come out alright. šŸ™‚ Of course they do!]
  2. TheĀ keĀ constant is the Coulomb constant and, from its definition keĀ = 1/4πε0, it’s easy to see how those two expressions are, in turn, equivalent with the third expression for α.
  3. The RKĀ constant is the so-called von Klitzing constant. Huh?Ā Yes. I know. I am pretty sure you’ve never everĀ heard of that one before. Don’t worry about it. It’s, quite simply, equal to RKĀ =Ā h/e2. Hence, substituting (and don’t forget that h = 2πħ) will demonstrate the equivalence of the fourth expression for α.
  4. Finally, theĀ reĀ factor is the classical electron radius, which is usually written as a function of me, i.e. the electron mass: reĀ = e2/4πε0mec2. Also note that this also implies that remeĀ = e2/4πε0c2. In words: the product of the electron mass and the electron radius is equal to some constant involving the electron (e), the electric constant (ε0), and c (the speed of light).

I am sure you’re under some kind of ‘formula shock’ now. But you should just take a deep breath and read on. The point to note is that all these very different things are all related through α.

So, again, whatĀ is that α really? Well… A strange number indeed. It’s dimensionless (so we don’t measure in kg, m/s, eVĀ·s or whatever) and it pops up everywhere. [Of course, you’ll say: “What’sĀ everywhere? This is the first timeĀ I‘ve heard of it!” :-)]

Well… Let me start by explaining the term itself.Ā The fine structure in the nameĀ refers to the splitting of the spectral lines of atoms. That’s a very fine structure indeed. šŸ™‚ We also have a so-called hyperfine structure. Both are illustrated below for theĀ hydrogenĀ atom. The numbers n,Ā J,Ā I, andĀ FĀ are quantum numbers used in the quantum-mechanical explanation of the emission spectrum, which is Ā also depicted below, but note that the illustration gives you the so-called Balmer series only, i.e. the colors in the visible light spectrum (there are many more ‘colors’ in the high-energy ultraviolet and the low-energy infrared range).

Fine_hyperfine_levels

Prism_5902760665342950662

To be precise:Ā (1)Ā n is the principal quantum number: here it takes the values 1 or 2, and we could say these are the principal shells;Ā (2) the S, P, D,… orbitals (which are usually written in lower case: s, p, d, f, g, h and i) correspond to the (orbital) angular momentum quantum numberĀ l = 0, 1, 2,…, so we could say it’s the subshell; (3) the J values correspond to theĀ so-called magnetic quantum number m, which goes from –lĀ toĀ +l; (4) the fourth quantum number is the spinĀ angular momentum s.Ā I’ve copied another diagram below so you see how it works, more or less, that is.

hydrogen spectrum

Now, our fine-structure constant is related to these quantum numbers. How exactly is a bit of a long story, and so I’ll just copy Wikipedia’s summary on this: ”Ā The gross structure of line spectra is the line spectra predicted by the quantum mechanics of non-relativistic electrons with no spin. For a hydrogenic atom, the gross structure energy levels only depend on the principal quantum number n. However, a more accurate model takes into account relativistic and spin effects, which break the degeneracy of the the energy levels and split the spectral lines. The scale of the fine structure splitting relative to the gross structure energies is on the order of (Zα)2, where Z is the atomic number and α is the fine-structure constant.” There you go.Ā You’ll say: so what? Well… Nothing. If you aren’t amazed by that, you should stop reading this.

It is an ‘amazing’ number, indeed, and, hence, it does quality for being “one of the greatest damn mysteries of physics”, as Feynman and/or Leighton put it.Ā Having said that,Ā I would not go as far as to write that it’s “a magic numberĀ that comes to us with no understanding by man.” In fact, I think Feynman/Leighton could have done a much better job when explaining what it’s all about. So, yes, I hope to do better than Leighton here and, as he’s still alive, I actually hope he reads this. šŸ™‚

The point is: α is not the only weird number. What’s particular about it, as a physical constant, is that it’s dimensionless, because it relates a number of otherĀ physical constants in such a way that the units fall away. Having said that, the Planck or Boltzmann constant are at least as weird.

So… What is this all about? Well… You’ve probably heard about the so-calledĀ fine-tuningĀ problem in physics and, if you’re like me, your first reaction will be to associate fine-tuning withĀ fine-structure. However, the two terms have nothing in common, except for four letters. šŸ™‚ OK. Well… I am exaggerating here. The two terms are actually related, to some extent at least, but let me explain how.

The term fine-tuning refers to the fact that all the parameters or constants in the so-called Standard Model of physics are, indeed, all related to each other in the way they are. We can’t sort of just turn the knob of one and change it, because everything falls apart then. So, in essence, the fine-tuning problem in physics is more like a philosophical question: why is the value of all these physical constants and parameters exactly what it is? So it’s like asking: could we change some of the ‘constants’ and still end up with the world we’re living in? Or, if it would be some different world, how would it look like? What ifĀ cĀ was some other number? What ifĀ keĀ or ε0Ā was some other number? In short, and in light of those expressions for α, we may rephrase the question as: why is α what is is?

Of course, that’s a question one shouldn’t try to answer before answering some other, more fundamental, question:Ā how many degrees of freedomĀ are there really?Ā Indeed, we just saw thatĀ keĀ and ε0Ā are intimately related through some equation, and other constants and parameters are related too. So the question is like: what are the ‘dependent’ and the ‘independent’ variables in this so-called Standard Model?

There is no easy answer to that question. In fact, one of the reasons why I find physics so fascinating is that one cannot easily answer such questions.Ā There are the obvious relationships, of course. For example, theĀ keĀ = 1/4πε0Ā relationship, and the context in which they are used (Coulomb’s Law) does, indeed, strongly suggest that both constants are actually part and parcel of the same thing. Identical, I’d say.Ā Likewise, the μ0ε0Ā = 1/c2Ā relation also suggests there’s only one degree of freedom here, just like there’s only one degree of freedom in that ω/kĀ =Ā cĀ relationship (if we set a value for ω, we have k, and vice versa). But… Well… I am not quite sure how to phrase this, but… What physical constants could be ‘variables’ indeed?

It’s pretty obvious that the various formulas for α cannotĀ answer that question: you could stare at them for days and weeks and months and years really, but I’d suggest you use your time to read more of Feynman’s realĀ LecturesĀ instead. šŸ™‚ One point that may help to come to terms with this question – to some extent, at least – is what I casually mentioned above already: the fine-structure constant is equal to the square of the electron charge expressed in Planck units: α =Ā eP2.

Now, that’sĀ veryĀ remarkable because Planck units are some kind of ‘natural units’ indeed (for the detail, see my previous post: among other things, it explains what these Planck units really are) and, therefore, it is quite tempting to think that we’ve actually got only oneĀ degree of freedom here: α itself. All the rest should follow from it.

[…]

It should…Ā But… Does it?

The answer is: yes and no. To be frank, it’s more no than yes because, as I noted a couple of times already, the fine-structure constant relates a lot of stuff but it’s surely not the only significant number in the Universe. For starters, I said thatĀ ourĀ E(A to B) formula has two ‘variables’:

  1. We have that complex numberĀ j, which, as mentioned, is equal to the electron chargeĀ expressed in Planck units. [In case you wonder why –ePĀ ā‰ˆ –0.08542455 is said to be an amplitude, i.e. aĀ complexĀ number or an ‘arrow’… Well… Complex numbersĀ includeĀ the real numbers and, hence, –0.08542455 is both real and complex. When combining ‘arrows’ or, to be precise, when multiplying some complex numberĀ with –0.08542455, we will (a) shrink the original arrow to about 8.5% of its original value (8.542455% to be precise) and (b) rotate it over an angle of plus or minus 180 degrees. In other words, we’ll reverse its direction. Hence, using Euler’s notation for complex numbers, we can write: –1 =Ā eiπ =Ā e–iπ and, hence, –0.085 = 0.085Ā·eiπ =Ā 0.085Ā·e–iĻ€. So, in short, yes, j is a complex number, or an ‘arrow’, if you prefer that term.]
  2. We also have someĀ some real numberĀ nĀ in the E(A to B) formula.Ā So what’s the n?Ā Well… Believe it or not, it’s the electron mass!Ā Isn’t that amazing?

You’ll say: “Well… Hmm… I suppose so.” But then you may – and actually should – alsoĀ wonder: the electron mass? In what units? Planck units again?Ā And are we talking relativistic mass (i.e. its total mass, including the equivalent mass of its kinetic energy) or its rest mass only? And we were talking α here, so can we relate it to α too, just like the electron charge?

These are all very good questions. Let’s start with the second one. We’re talking ratherĀ slow-moving electrons here, so the relativistic mass (m) and its rest mass (m0) is more or less the same. Indeed, the Lorentz factor γ in the m = γm0Ā equation isĀ veryĀ close to 1 for electrons moving at their typical speed. So… Well… That question doesn’t matter very much.Ā Really?Ā Yes. OK. Because you’re doubting, I’ll quickly show it to you.Ā What is their ‘typical’ speed?

We know we shouldn’t attach too much importance to the concept of an electron in orbit around some nucleus (we know it’s not like some planet orbiting around some star) and, hence, to the concept of speed or velocity (velocity is speed with direction) when discussing an electron in an atom. The concept of momentumĀ (i.e. velocity combined with mass or energy) is much more relevant.Ā There’s a very easy mathematical relationship that gives us some clue here: the Uncertainty Principle. In fact, we’ll use the Uncertainty Principle to relate the momentum of an electron (p) to the so-called Bohr radius r (think of it as the size of a hydrogen atom) as follows: p ā‰ˆ ħ/r. [I’ll come back on this in a moment, and show you why this makes sense.]

Now we also know its kinetic energy (K.E.) is mv2/2, which we can write as p2/2m. Substituting our p ā‰ˆ ħ/r conjecture, we get K.E. =Ā mv2/2 = ħ2/2mr2. This is equivalent to m2v2Ā = ħ2/r2Ā (just multiply both sides with m). From that, we get vĀ = ħ/mr. Now, one of the many relations we can derive from the formulas for the fine-structure constant is reĀ = α2r. [I haven’t showed you that yet, but I will shortly. It’s a really amazing expression. However, as for now, just accept it as a simple formula for interim use in this digression.] Hence, r =Ā re/α2. The reĀ factor in this expression is the so-called classical electron radius. So we can now writeĀ vĀ = ħα2/mre. Let’s now throw cĀ in: v/c = α2ħ/mcre. However, from that fifth expression for α, we know that ħ/mcreĀ = α, so we get v/c = α. We have another amazing result here: the v/c ratio for an electron (i.e. its speed expressed as a fraction of the speed of light) is equal to that fine-structure constant α. So that’s aboutĀ 1/137, so that’s lessĀ than 1% of the speed of light. Now… I’ll leave it to you to calculate the Lorentz factor γ but… Well… It’s obvious that it will beĀ veryĀ close to 1. šŸ™‚ Hence, the electron’s speed – however we want to visualize that – doesn’t matter much indeed, so we should not worry about relativistic corrections in the formulas.

Let’s now look at the question in regard to the Planck units. If you know nothing at all about them, I would advise you to read what I wrote about them in my previous post. Let me just note we get those Planck units by equating not less thanĀ five fundamental physical constants to 1, notably (1) the speed of light, (2) Planck’s (reduced) constant, (3) Boltzmann’s constant, (4) Coulomb’s constant and (5) Newton’s constant (i.e. the gravitational constant). Hence, we have a set of five equations here (cĀ = ħ = kBĀ = keĀ = G = 1), and so we can solve that to get the five Planck units, i.e. the Planck length unit, the Planck time unit, the Planck mass unit, the Planck energy unit, the Planck charge unit and, finally (oft forgotten), the Planck temperature unit. Of course, you should note that all mass and energy units areĀ directlyĀ related because of the mass-energy equivalence relationĀ E = mc2, which simplifies to E = m if cĀ is equated to 1. [I could also say something about the relation between temperature and (kinetic) energy, but I won’t, as it would only further confuse you.]

Now, you may or may not remember thatĀ the Planck time and length units are unimaginably small, but that the Planck mass unit is actually quite sizable—at the atomic scale, that is. Indeed, the Planck mass isĀ something huge,Ā like the mass of an eyebrow hair, or a flea egg. Is that huge? Yes. Because if you’d want to pack it in a Planck-sized particle, it would make for a tiny black hole. šŸ™‚ No kidding. That’s the physical significance of the Planck mass and the Planck length and, yes, it’s weird. šŸ™‚

Let me give you some values.Ā First, the Planck mass itself:Ā it’sĀ aboutĀ 2.1765Ɨ10āˆ’8Ā kg. Again, if you think that’s tiny, think again. From the E = mc2Ā equivalence relationship, we get that this is equivalent to 2 giga-joule, approximately. Just to give an idea, that’s like the monthly electricity consumption of an average American family. So that’s huge indeed! šŸ™‚Ā [Many people think that nuclear energy involves the conversion of mass into energy, but the story is actually more complicated than that. In any case… I need to move on.]

Let me now give you the electron mass expressed in the Planck mass unit:

  1. Measured in our old-fashioned super-sized SI kilogram unit, the electron mass is meĀ = 9.1Ɨ10–31Ā kg.
  2. The Planck mass is mPĀ = 2.1765Ɨ10āˆ’8Ā kg.
  3. Hence, the electron mass expressed in Planck units is mePĀ = me/mPĀ =Ā (9.1Ɨ10–31Ā kg)/(2.1765Ɨ10āˆ’8Ā kg)Ā = 4.181Ɨ10āˆ’23.

We can, once again, write that as some function of the fine-structure constant.Ā More specifically, we can write:

meP = α/reP = α/α2rP  = 1/αrP

So… Well… Yes: yetĀ another amazing formula involving α.

In this formula, we haveĀ rePĀ andĀ rP, which are the (classical) electron radius and the Bohr radius expressed in Planck (length) units respectively. So you can see what’s going on here: we have all kinds of numbers here expressed in Planck units: a charge, a radius, a mass,…Ā And we can relate all of them to the fine-structure constant.Ā 

Why? Who knows? I don’t. As Leighton puts it: that’s just the way “God pushed His pencil.” šŸ™‚

Note that the beauty of natural units ensures that we get the same number for the (equivalent) energy of an electron. Indeed, from the E = mc2Ā relation, we know the mass of an electron can also be written as 0.511 MeV/c2. Hence, the equivalent energy is 0.511 MeV (so that’s, quite simply, the same number but without the 1/c2Ā factor). Now, the Planck energy EPĀ (in eV) is 1.22Ɨ1028Ā eV, so we get EePĀ = Ee/EPĀ = (0.511Ɨ106Ā eV)/(1.22Ɨ1028Ā eV) = 4.181Ɨ10āˆ’23. So it’s exactly the same as the electron massĀ expressed in Planck units.Ā Isn’t that nice? šŸ™‚

Now, are all these numbers dimensionless, just like α? The answer to that question is complicated. Yes, and… Well… No:

  1. Yes. They’re dimensionless because they measure something in natural units, i.e. Planck units, and, hence, that’s some kind of relativeĀ measure indeed so… Well… Yes, dimensionless.
  2. No. They’re not dimensionless because they do measureĀ something, like a charge, a length, or a mass, and when you chose some kind of relativeĀ measure, you still need to define some gauge, i.e. some kind of standard measure. So there’s some ‘dimension’ involved there.

So what’s the final answer? Well… The Planck units are notĀ dimensionless. All we can say is that they are closely related, physically. I should also add that we’ll use the electron charge and mass (expressed in Planck units) in our amplitude calculations as a simple (dimensionless) number between zero and one. So the correct answer to the question as to whether these numbers have any dimension is: expressing someĀ quantitiesĀ in Planck units sort ofĀ normalizesĀ them, so we can use them directly in dimensionless calculations, like when we multiply and add amplitudes.

Hmm…Ā Well…Ā I can imagine you’re not very happy with this answer but it’s the best I can do. Sorry. I’ll letĀ youĀ further ponder that question.Ā I need to move on.Ā Ā 

Note thatĀ that 4.181Ɨ10āˆ’23Ā is still a very small number (23 zeroes after the decimal point!), even if it’s like 46 million times larger than the electron mass measured in our conventional SI unit (i.e. 9.1Ɨ10–31Ā kg). Does such small number make any sense? The answer is: yes, it does. When we’ll finally start discussing that E(A to B) formula (I’ll give it to you in a moment), you’ll see that a very small number for n makes a lot of sense.

Before diving into it all,Ā let’s first see if that formula for that alpha, that fine-structure constant, still makes sense with me expressed in Planck units. Just to make sure. šŸ™‚ To do that, we need to use the fifth (last) expression for a, i.e. the one with reĀ in it. Now, in my previous post, I also gave some formula for re: reĀ = e2/4πε0mec2, which we can re-write as remeĀ = e2/4πε0c2. If we substitute that expression for remeĀ  in the formula for α, we can calculate α from the electron charge, which indicates both the electron radius and its mass are not some random God-given variable, or “some magic number that comes to us with no understanding by man“, as Feynman – well… Leighton, I guess – puts it. No. They are magic numbers alright, one related to another through the equally ‘magic’ number α, but so I doĀ feel we actually canĀ create some understanding here.

At this point, I’ll digress once again, and insert some quick back-of-the-envelope argument from Feynman’s very serious CaltechĀ Lectures on Physics, in which, as part of the introduction to quantum mechanics, he calculates the so-called BohrĀ radius from Planck’s constant h. Let me quickly explain: the Bohr radius is, roughly speaking, the size of the simplest atom, i.e. an atom with one electron (so that’s hydrogen really). So it’s not the classical electron radius re. However, both are also related to that ‘magical number’ α. To be precise, if we write the Bohr radius as r, then reĀ = α2rĀ ā‰ˆ 0.000053… timesĀ r, which we can re-write as:

α = √(re /r) = (re /r)1/2

So that’sĀ yet another amazing formula involving the fine-structure constant. In fact, it’s the formula I used as an ‘interim’ expression to calculate the relative speed of electrons. I just used it without any explanation there, but I am coming back to it here. Alpha again…

Just think about it for a while. In case you’d still doubt the magic of that number, let me write what we’ve discovered so far:

(1) α is the square of the electron charge expressed in Planck units: α = eP2.

(2) α is the square root of the ratio of (a) the classical electron radius and (b) the Bohr radius: α = √(reĀ /r). You’ll see this more often written asĀ reĀ = α2r. Also note that this is an equation that doesĀ notĀ depend on the units, in contrast to equation 1 (above), and 4 and 5 (below), which require you to switch to Planck units. It’s the square of a ratio and, hence, the units don’t matter. They fall away.

(3) α is the (relative) speed of an electron: α = v/c. [The relative speed is the speed as measured against the speed of light. Note that the ‘natural’ unit of speed in the Planck system of units is equal to c. Indeed, if you divide one Planck length by one Planck time unit, you get (1.616Ɨ10āˆ’35Ā m)/(5.391Ɨ10āˆ’44Ā s) =Ā cĀ m/s. However, this is another equation, just like (2), that does notĀ depend on the units: we can express v and c in whatever unit we want, as long we’re consistent and express both in the same units.]

(4) Finally – I’ll show you in a moment – α is also equal to the product of (a) the electron mass (which I’ll simply write as meĀ here) and (b) the classical electron radius reĀ (if both are expressed in Planck units): α =Ā meĀ·re. Now IĀ thinkĀ that’s, perhaps, theĀ mostĀ amazing of all of the expressions for α. If you don’t think that’s amazing, I’d really suggest you stop trying to study physics. šŸ™‚

Note that, from (2) and (4), we find that:

(5) The electron mass (in Planck units) is equal me = α/re = α/α2r = 1/αr. So that gives us an expression, using α once again, for the electron mass as a function of the Bohr radius r expressed in Planck units.

Finally, we can also substitute (1) in (5) to get:

(6) The electron mass (in Planck units) is equal to me = α/re  = eP2/re. Using the Bohr radius, we get me = 1/αr = 1/eP2r.

So… As you can see, this fine-structure constant really links ALLĀ of the fundamental properties of the electron: its charge, its radius, its distance to the nucleus (i.e. the Bohr radius), its velocity, its mass (and, hence, its energy),… In short,

IT IS ALL IN ALPHA!

NowĀ thatĀ should answer the question in regard to the degrees of freedom we have here, doesn’t it? It looks like we’ve got only one degree of freedom here. Indeed, if we’ve gotĀ some value for α, then we’ve have the electron charge, and from the electron charge, we can calculate the Bohr radius r (as I will show below), and if we have r, we have meĀ andĀ re. And then we can also calculate v, which gives us its momentum (mv) and its kinetic energy (mv2/2). In short,

ALPHA GIVES US EVERYTHING!

Isn’t that amazing? Hmm… You should reserve your judgment as for now, and carefully go over all of the formulas above and verify my statement. If you do that, you’ll probably struggle to find the Bohr radius from the charge (i.e. from α). So let me show you how you do that, because it will also show you whyĀ you should, indeed, reserve your judgment. In other words, I’ll show you why alpha does NOT give us everything! The argument below will, finally, prove some of the formulas that I didn’t prove above. Let’s go for it:

1. If we assume that (a) an electron takes some space – which I’ll denote by rĀ šŸ™‚ – and (b) that it has some momentum p because of its mass m and its velocity v, then the Ī”xĪ”p = ħ relation (i.e. the Uncertainty Principle in its roughest form) suggests that the order of magnitude of r and p should be related in the very same way. Hence, let’s just boldly write r ā‰ˆ ħ/p and see what we can do with that. So we equate Ī”x with r and Ī”p with p. As Feynman notes, this is really more like a ‘dimensional analysis’ (he obviously means something very ‘rough’ with that) and so we don’t care about factors like 2 or 1/2. [Indeed, note that the more precise formulation of the Uncertainty Principle is σxσp ≄ ħ/2.]Ā In fact, we didn’t even bother to define r very rigorously. We just don’t care about precise statements at this point. We’re only concerned about orders of magnitude. [If you’re appalled by the rather rude approach, I am sorry for that, but just try to go along with it.]

2. From our discussions on energy, we know that the kinetic energy is mv2/2, which we can write as p2/2m so we get rid of the velocity factor. [Why? Because we can’t really imagine what it is anyway. As I said a couple of times already, we shouldn’t think of electrons as planets orbiting around some star. That model doesn’t work.] So… What’s next? Well… Substituting our p ā‰ˆ ħ/r conjecture, we get K.E. = ħ2/2mr2. So that’s a formula for the kinetic energy. Next is potential.

3.Ā Unfortunately, the discussion on potential energy is a bit more complicated. You’ll probably remember that we had an easy and very comprehensible formula for the energy that’s needed (i.e. the work that needs to be done) to bring two charges together from a large distance (i.e. infinity). Indeed, we derived that formula directly from Coulomb’s Law (and Newton’s law of force) and it’s U = q1q2/4πε0r12. [If you think I am going too fast, sorry, please check for yourself by reading my other posts.] Now, we’re actually talking about the size of an atomĀ hereĀ in my previous post, so one charge is the proton (+e) and the other is the electron (–e), so the potential energy is U = P.E. = –e2/4πε0r, with rĀ the ‘distance’ between the proton and the electron—so that’s the Bohr radius we’re looking for!

[In case you’re struggling a bit with those minus signs when talking potential energy  – I am not ashamed to admit I did! – let me quickly help you here. It has to do with our reference point: the reference point for measuring potential energy is at infinity, and it’s zero there (that’s just our convention). Now, to separate the proton and the electron, we’d have to do quite a lot of work. To use an analogy: imagine we’re somewhere deep down in a cave, and we have to climb back to the zero level. You’ll agree that’s likely to involve some sweat, don’t you? Hence, the potential energy associated with us being down in the cave is negative. Likewise, if we write the potential energy between the proton and the electron as U(r), and the potential energy at the reference point as U(āˆž) = 0, then the work to be done to separate the charges, i.e. the potential differenceĀ U(āˆž) – U(r), will be positive. So U(āˆž) – U(r) = 0 – U(r)Ā > 0 and, hence, U(r) <Ā 0. If you still don’t ‘get’ this, think of the electron being in some (potential) well, i.e.Ā belowĀ the zero level, and so it’s potential energy isĀ lessĀ than zero. Huh?Ā Sorry. I have to move on. :-)]

4. We can now write the total energy (which I’ll denote by E, but don’t confuse it with the electric field vector!) as

E = K.E. + P.E. =  ħ2/2mr2 – e2/4πε0r

Now, the electron (whatever it is) is, obviously, in some kind of equilibrium state. Why is that obvious? Well… Otherwise our hydrogen atom wouldn’t or couldn’t exist. šŸ™‚ Hence, it’s in some kind of energy ‘well’ indeed, at the bottom. Such equilibrium point ‘at the bottom’ is characterized by its derivative (in respect to whatever variable) being equal to zero. Now, the only ‘variable’ here isĀ rĀ (all the other symbols are physical constants), so we have to solve for dE/dr = 0. Writing it all out yields:

dE/dr = –ħ2/mr3Ā + e2/4πε0r2Ā = 0 ⇔ r =Ā 4πε0ħ2/me2

You’ll say: so what? Well… We’ve got a nice formula for the Bohr radius here, and we got it in no time! šŸ™‚ But the analysis was rough, so let’s check if it’s any good by putting the values in:

r =Ā 4πε0h2/me2

= [(1/(9Ɨ109) C2/NĀ·m2)Ā·(1.055Ɨ10–34Ā JĀ·s)2]/[(9.1Ɨ10–31Ā kg)Ā·(1.6Ɨ10–19Ā C)2]

= 53Ɨ10–12Ā m = 53 pico-meter (pm)

So what? Well… Double-check it on the Internet: the Bohr radius is, effectively, about 53 trillionthsĀ of a meter indeed! So we’re right on the spot!Ā 

[In case you wonder about the units, note that mass is a measure of inertia: one kg is the mass of an object which, subject to a force of 1 newton, will accelerate at the rate of 1 m/sĀ per second. Hence, we write F = mĀ·a, which is equivalent to m = F/a. Hence, the kg, as a unit, is equivalent to 1 N/(m/s2). If you make this substitution, we get r in the unit we want to see: [(C2/NĀ·m2)Ā·(N2Ā·m2Ā·s2)/[(NĀ·s2/m)Ā·C2] = m.]

Moreover, if we take that value for rĀ and put it in the (total) energy formula above, we’d find that the energy of the electron is –13.6 eV. [Don’t forget to convert from joule to electronvolt when doing the calculation!] Now you can check that on the Internet too: 13.6 eV is exactlyĀ the amount of energy that’s needed to ionize a hydrogen atom (i.e. the energy that’s needed to kick the electron out of that energy well)!

Waw ! Isn’t it great that such simple calculations yield such great results? šŸ™‚ [Of course, you’ll note that the omission of the 1/2 factor in the Uncertainty Principle was quite strategic. :-)] Using theĀ r =Ā 4πε0ħ2/me2Ā formula for the Bohr radius, you can now easily check the reĀ = α2rĀ formula. You should find what we jotted down already: the classical electron radius is equal to reĀ = e2/4πε0mec2. To be precise,Ā reĀ = (53Ɨ10–6)Ā·(53Ɨ10–12m) = 2.8Ɨ10–15Ā m. Now that’s again something you should check on the Internet. Guess what? […] It’s right on the spot again. šŸ™‚

We can now also check that α = mĀ·reĀ formula: α = mĀ·reĀ =Ā 4.181Ɨ10āˆ’23Ā times… Hey! Wait! We have to expressĀ re in Planck units as well, of course! Now, (2.81794Ɨ10–15Ā m)/(1.616Ɨ10–35Ā m) ā‰ˆ 1.7438 Ɨ1020. So now we getĀ 4.181Ɨ10āˆ’23Ā timesĀ 1.7438Ɨ1020Ā = 7.29Ɨ10–3Ā = 0.00729Ā ā‰ˆ 1/137. Bingo! We got the magic number once again. šŸ™‚

So… Well… Doesn’t that confirm we actually do have it all with α?

Well… Yes and no… First, youĀ should note that I had to useĀ hĀ in that calculation of the Bohr radius. Moreover, the other physical constants (most notably c and the Coulomb constant) were actually there as well, ‘in the background’ so to speak, because one needs them to derive the formulas we used above. And then we have the equations themselves, of course, most notably that Uncertainty Principle… So… Well…

It’s not like God gave us one number only (α) and that all the rest flows out of it. We have a whole bunch of ‘fundamental’ relations and ‘fundamental’ constants here.

Having said that, it’s true that statement still does not diminish the magic of alpha.

Hmm… Now you’ll wonder: how many? How many constants do we need in all of physics?

Well… I’d say, you should not only ask about the constants: you should also ask about the equations: how many equations do we need in all of physics? [Just for the record, I had to smile when the Hawking of the movie says that he’s actually looking forĀ one formula that sums up all of physics.Ā Frankly, that’s a nonsensical statement. Hence, I think the real Hawking never said anything like that. Or, if he did, that it was one of those statements one needs to interpret veryĀ carefully.]

But let’s look at a few constants indeed. For example, if we have c, hĀ and α, then we can calculate the electric charge e and, hence, the electric constant ε0Ā = e2/2αhc. From that, we get Coulomb’s constant ke, because keĀ is defined as 1/4πε0… But…

Hey! Wait a minute!Ā How do weĀ knowĀ that keĀ = 1/4πε0?Ā Well… From experiment.Ā But…Ā Yes? That means 1/4Ļ€ is some fundamental proportionality coefficient too, isn’t it?

Wow! You’re smart. That’s a good and valid remark. In fact, we use the so-calledĀ reduced Planck constant ħ in a number of calculations, and so that involves a 2Ļ€ factor too (ħ = h/2Ļ€). Hence… Well… Yes, perhaps we should consider 2Ļ€ as some fundamental constant too! And, then, well… Now that I think of it, there’s a few other mathematical constants out there, like Euler’s numberĀ e, for example, which we use in complex exponentials.

?!?

I am joking, right? I amĀ not sayingĀ that 2Ļ€ andĀ Euler’s number are fundamental ‘physical’ constants, am I? [Note thatĀ it’s a bit of a nuisance we’re also using the eĀ symbol for Euler’s number, but so we’re not talking the electron charge here: we’re talking thatĀ 2.71828…etc number that’s used in so-called ‘natural’ exponentials and logarithms.]

Well… Yes and no. They’re mathematicalĀ constants indeed, rather than physical, but… Well… I hope you get my point.Ā What I want to show here, is that it’s quite hard to say what’s fundamental and what isn’t. We can actually pick and choose a bit among all those constants and all those equations. As one physicist puts its: it depends on how we slice it. The one thing we know for sure is that a great many things are related, in a physical way (α connects all of the fundamental properties of the electron, for example) and/or in a mathematicalĀ way (2Ļ€ connects not only the circumference of the unit circle with the radius but quite a few other constants as well!), but… Well… What to say?Ā It’s a tough discussion and I am not smart enough to give you an unambiguous answer.Ā From what I gather on the Internet, when looking at the wholeĀ Standard Model (including the strong force, the weak force and the Higgs field), we’ve got a few dozen physical ‘fundamental’ constants, and then a few mathematical ones as well.

That’s a lot, you’ll say. Yes. At the same time, it’s not an awful lot. Whatever number it is, it does raise a very fundamental question: why are they what they are? That brings us back to that ‘fine-tuning’ problem. Now, I can’t make this post too long (it’s way too long already), so let me just conclude this discussion by copying Wikipedia on that question, because what it hasĀ on this topic is not so bad:

“Some physicists have explored the notion that if the physical constants had sufficiently different values, our Universe would be so radically different that intelligent life would probably not have emerged, and that our Universe therefore seems to be fine-tuned for intelligent life. The anthropic principle states a logical truism: the fact of our existence as intelligent beings who can measure physical constants requires those constants to be such that beings like us can exist.“

I like this. But the article then adds the following, which I do not like so much, because I think it’s a bit too ‘frivolous’:

“There are a variety of interpretations of the constants’ values, including that of a divine creator (the apparent fine-tuning is actual and intentional), or that ours is one universe of many in a multiverseĀ (e.g.Ā the many-worlds interpretation of quantum mechanics), or even that, if information is an innate property of the universe and logically inseparable from consciousness, a universe without the capacity for conscious beings cannot exist.”

Hmm… As said, I am quite happy with the logical truism: we are there because alpha (and a whole range of other stuff) is what it is, and we can measure alpha (and a whole range of other stuff) as what it is, because… Well… Because we’re here. Full stop.Ā As for the ‘interpretations’, I’ll let you think about that for yourself. šŸ™‚

I need to get back to the lesson. Indeed, this was just a ‘digression’. My post was about the three fundamental events or actions in quantum electrodynamics, and so I was talking about that E(A to B) formula. However, I had to do that digression on alpha to ensure you understand what I want to write about that. So let me now get back to it. End of digression. šŸ™‚

The E(A to B) formula

Indeed, I must assume that, with all these digressions, you are truly despairing now. Don’t. We’re there! We’re finally ready for theĀ E(A to B) formula! Let’s go for it.

We’ve now got those two numbers measuring the electron charge and the electron mass in Planck unitsĀ respectively. They’re fundamental indeed and so let’s loosen up on notation and just write them as e and m respectively. Let me recap:

1. The value of e is approximately –0.08542455, and it corresponds to the so-called junction number j, which is the amplitude for an electron-photon coupling. When multiplying it with another amplitude (to find the amplitude for an event consisting of two sub-events, for example), it corresponds to a ‘shrink’ to less than one-tenth (something like 8.5% indeed, corresponding to the magnitudeĀ of e) and a ‘rotation’ (or a ‘turn’) over 180 degrees, as mentioned above.

Please note what’s going on here: we have a physical quantity, the electron charge (expressed in Planck units), and we use it in a quantum-mechanical calculation as a dimensionless (complex) number, i.e. as an amplitude. So… Well… That’s what physicists mean when they say that the charge of some particle (usually the electric charge but, in quantum chromodynamics, it will be the ‘color’ charge of a quark) is a ‘coupling constant’.

2.Ā We also have m, the electron mass, and we’ll use in the same way, i.e. as some dimensionless amplitude. As compared to j, it’s is a veryĀ tiny number: approximatelyĀ 4.181Ɨ10āˆ’23. So if you look at it as an amplitude, indeed, then it corresponds to an enormous ‘shrink’ (but no turn) of the amplitude(s) that we’ll be combining it with.

So… Well… How do we do it?

Well… At this point, Leighton goes a bit off-track. Just a little bit. šŸ™‚ From what he writes, it’s obvious that he assumes the frequency (or, what amounts to the same, the de BroglieĀ wavelength)Ā of an electron is just like the frequency of a photon. Frankly, I just can’t imagine why and how Feynman let this happen. It’s wrong. Plain wrong. As I mentioned in my introduction already, an electron traveling through space is not like a photon traveling through space.

For starters, an electron is much slower (because it’s a matter-particle: hence, it’s got mass). Secondly, theĀ de BroglieĀ wavelength and/or frequency of an electron is not like that of a photon.Ā For example, if we take an electron and a photon having the same energy, let’s say 1 eV (that corresponds to infrared light), then the de BroglieĀ wavelength of the electronĀ will be 1.23 nano-meter (i.e. 1.23 billionths of a meter). Now that’s about one thousand times smaller than the wavelength of our 1 eV photon, which is about 1240 nm.Ā You’ll say: how is that possible? If they have the same energy, then the f = E/h and ν = E/h should give the same frequency and, hence, the same wavelength, no?

Well… No! Not at all!Ā Because an electron, unlike the photon, has a rest mass indeed – measured as not less than 0.511 MeV/c2, to be precise (note the rather particular MeV/c2 unit: it’s from the E = mc2 formula) – one should use a different energy value! Indeed, we should include the rest mass energy, which is 0.511 MeV. So,Ā almost all of the energy here is rest mass energy!Ā There’s also another complication. For the photon, there is an easy relationship between the wavelength and the frequency:Ā it has no mass and, hence, all its energy is kinetic, or movement so to say,Ā and so we can use that ν = E/h relationship to calculate its frequency ν: it’s equal to ν = E/h = (1 eV)/(4.13567Ɨ10–15Ā eVĀ·s)Ā ā‰ˆ 0.242Ɨ1015Ā Hz = 242Ā tera-hertz (1 THz = 1012Ā oscillations per second). Now, knowing that light travels at the speed of light, we can check the result by calculating the wavelength using the Ī» = c/ν relation. Let’s do it: (2.998Ɨ108Ā m/s)/(242Ɨ1012Ā Hz) ā‰ˆ 1240 nm. So… Yes, done!

But so we’re talking photons here.Ā For the electron, the story is much more complicated. That wavelength I mentioned was calculated using the other of the two de BroglieĀ relations:Ā Ī» = h/p. So that uses the momentumĀ of the electron which, as you know, is the product of its mass (m) and its velocity (v): p = mv. You can amuse yourself and check if you find the same wavelength (1.23 nm): you should! From the other de Broglie relation, f = E/h, you can also calculate its frequency: for an electron moving at non-relativistic speeds, it’s about 0.123Ɨ1021Ā Hz, so that’s like 500,000 times the frequency of the photon we we’re looking at! When multiplying the frequency and the wavelength, we should get its speed. However, that’s where we get in trouble. Here’s theĀ problem withĀ matter waves: they have a so-called group velocity and a so-called phase velocity. The idea is illustrated below: the green dot travels with the wave packet – and, hence, its velocity corresponds to the group velocity – while the red dot travels with the oscillation itself, and so that’s the phase velocity. [You should also remember, of course, that the matter wave is some complex-valuedĀ wavefunction, so we have both a real as well as an imaginary part oscillating and traveling through space.]

Wave_group (1)

To be precise, the phase velocity will be superluminal. Indeed, using the usual relativistic formula, we can write that p = γm0v and E = γm0c2, with v the (classical) velocity of the electron and cĀ what it always is, i.e. the speed of light. Hence, Ī» = h/γm0vĀ andĀ fĀ = γm0c2/h, and so Ī»f = c2/v. Because v is (much) smaller than c, we get a superluminal velocity. However, that’s the phase velocity indeed, not the group velocity, which corresponds to v. OK… I need to end this digression.

So what? Well, to make a long story short, the ‘amplitude framework’ for electrons is differerent. Hence, theĀ story that I’ll be telling here is different from what you’ll read in Feynman’s QED. I will use his drawings, though, and his concepts. Indeed, despite my misgivings above, the conceptual framework is sound, and so the corrections to be made are relatively minor.

So… We’re looking at E(A to B), i.e. theĀ amplitude for an electronĀ to go from point A to B in spacetime, and I said the conceptual framework is exactly the same as that for a photon. Hence, the electron can follow any path really. It mayĀ go in a straight line and travel at a speed that’s consistent with what we know of its momentum (p), but it may also follow other paths.Ā So, just like the photon, we’ll have some so-called propagatorĀ function, which gives youĀ amplitudes based on the distance in space as well as in the distance in ‘time’ between two points. Now, Ralph Leighton identifies that propagator function with the propagator function for the photon, i.e. P(A to B), but that’s wrong: it’s not the same.

The propagator function for an electron depends on its mass and its velocity, and/or on the combination of both (like it momentum p = mvĀ and/or its kineticĀ energy: K.E. =Ā mv2Ā = p2/2m). So we have a different propagator function here. However, I’ll use the same symbol for it: P(A to B).

So, the bottom line is that, because of the electron’s mass (which, remember, is a measure for inertia), momentum and/or kinetic energy (which, remember, are conserved in physics), theĀ straight line is definitelyĀ the most likely path, butĀ (big but!), just like the photon, the electron may follow some other path as well.

So how do we formalize that?Ā Let’s first associate an amplitude P(A to B) with an electron traveling from point A to B in a straight line and in a time that’s consistent with its velocity. Now, as mentioned above, the P here stands for propagator function, not for photon, so we’re talking a different P(A to B) here than that P(A to B) function we used for the photon. Sorry for the confusion. šŸ™‚ The left-hand diagram below then shows what we’re talking about: it’s the so-called ‘one-hop flight’, and so that’s what the P(A to B) amplitude is associated with.

Diagram 1Now, the electron can follow other paths. For photons, we said the amplitude depended on the spacetime interval I: when negative or positive (i.e. paths that areĀ notĀ associated with the photon traveling in a straight line and/or at the speed of light), the contribution of those paths to theĀ finalĀ amplitudes (or ‘final arrow’, as it was called) was smaller.

For an electron, we have something similar, but it’s modeled differently. We say the electron could take a ‘two-hop flight’ (via point C or C’), or a ‘three-hop flight’ (via D and E) from point A to B. Now, it makes sense that these paths should be associated with amplitudes that are much smaller. Now that’s where that n-factor comes in. We just put some real number n in the formula for the amplitude for anĀ electron to go from A to B via C, which we write as:

P(A to C)āˆ—n2āˆ—P(C to B)

Note what’s going on here. We multiply two amplitudes, P(A to C) and P(C to B), which is OK, because that’s what the rules of quantum mechanics tell us: if an ‘event’ consists of two sub-events, we need to multiply the amplitudes (not the probabilities) in order to get the amplitude that’s associated withĀ bothĀ sub-events happening. However, we add an extra factor: n2. Note that it must be some very small number because we have lots of alternative paths and, hence, they should not be very likely!Ā So what’s the n? And why n2Ā instead of just n?

Well… Frankly, I don’t know. Ralph Leighton boldly equates n to the mass of the electron. Now, because he obviously means the mass expressed in Planck units, that’s the same as saying n is the electron’s energy (again, expressed in Planck’s ‘natural’ units), so n should be that number m = mePĀ = EePĀ = 4.181Ɨ10āˆ’23. However, I couldn’t find any confirmation on the Internet, or elsewhere, of the suggested n = m identity, so I’ll assume n = m indeed, but… Well… Please check for yourself. It seems the answer is to be found in a mathematical theory that helps physicists to actually calculate j and n from experiment. It’s referred to asĀ perturbation theory, and it’s the next thing on my study list. As for now, however, I can’t help you much.Ā I can only note that theĀ equation makes sense.

Of course, it does: inserting a tiny little number n, close to zero, ensures that those other amplitudes don’t contribute too much to the final ‘arrow’. And it also makes a lot of sense toĀ associate it with the electron’s mass: if mass is a measure of inertia, then it should be some factor reducingĀ the amplitude that’s associated with the electron following such crooked path. So let’s go along with it, and see what comes out of it.

A three-hop flight is even weirder and uses that n2Ā factor two times:

P(A to E)āˆ—n2āˆ—P(E to D)āˆ—n2āˆ—P(D to B)

So we have an (n2)2Ā = n4Ā factor here, which is good, because two hops should be much less likely than one hop. So what do we get? Well… (4.181Ɨ10āˆ’23)4Ā ā‰ˆ 305Ɨ10āˆ’92. Pretty tiny, huh? šŸ™‚Ā Of course, any point in space is a potential hop for the electron’s flight from point A to B and, hence, there’s a lot of paths and a lot of amplitudes (or ‘arrows’ if you want), which, again, is consistent with a very tiny value for n indeed.

So, to make a long story short, E(A to B) will be a giant sum (i.e. some kind of integral indeed) of a lot of different ways an electron can go from point A to B. It will be aĀ seriesĀ of termsĀ P(A to E) +Ā P(A to C)āˆ—n2āˆ—P(C to B) +Ā P(A to E)āˆ—n2āˆ—P(E to D)āˆ—n2āˆ—P(D to B) + …Ā for all possible intermediate points C, D, E, and so on.

What about the j? The junction number of coupling constant. How does that show up in the E(A to B) formula? Well… Those alternative paths with hops here and there are actually the easiest bit of the whole calculation. Apart from taking some strange path, electrons can also emit and/or absorb photons during the trip. In fact, they’re doing that constantly actually. Indeed, the image of an electron ‘in orbit’ around the nucleus is that of an electron exchanging so-called ‘virtual’ photonsĀ constantly, as illustrated below. So our image of an electron absorbing and then emitting a photon (see the diagram on the right-hand side) is really like the tiny tip of a giant iceberg: most of what’s going on is underneath!Ā So that’s where our junction number j comes in, i.e. the charge (e) of the electron.

So, when you hear that a coupling constant is actually equal to the charge, then this is what it means: you should just note it’s the chargeĀ expressed in Planck units. But it’s a deep connection, isn’t? When everything is said and done, a charge is somethingĀ physical, but so here, in these amplitude calculations, it just shows up as some dimensionless negative number, used in multiplications and additions of amplitudes. Isn’t that remarkable?

d2 d3

The situation becomes even more complicated when more than one electron is involved. For example, two electrons can go in a straight line from point 1 and 2 to point 3 and 4 respectively, but there’s two ways in which this can happen, and they might exchange photons along the way, as shown below. If there’s twoĀ alternativeĀ ways in which one event can happen, you know we have to add amplitudes, rather than multiply them. Hence, the formula for E(A to B) becomes even more complicated.

D5d4

Moreover, a single electron may first emit and then absorb a photon itself, so there’s no need for other particles to be there to have lots of j factors in our calculation. In addition, that photon may briefly disintegrate into an electron and a positron, which then annihilate each other to again produce a photon: in case you wondered, that’s what those little loops in those diagrams depicting the exchange of virtual photons is supposed to represent. So, everyĀ single junction (i.e. every emission and/or absorption of a photon) involves a multiplication with that junction number j, so if there are two couplings involved, we have a j2Ā factor, and so that’s 0.085424552Ā = α ā‰ˆ 0.0073. Four couplings implies a factor ofĀ 0.085424554Ā ā‰ˆ 0.000053.

Just as an example,Ā I copy two diagrams involving four, five or six couplings indeed. They all have some ‘incoming’ photon, because Feynman uses them to explain something else (the so-called magnetic moment of a photon), but it doesn’t matter: the same illustrations can serve multiple purposes.

d6 d7

Now, it’s obvious that the contributionsĀ of the alternatives with many couplings add almost nothing to the final amplitude – just like the ‘many-hop’ flights add almost nothing – but… Well… As tiny as these contributions are, they are all there, and so they all have to be accounted for. So… Yes. YouĀ can easily appreciate how messy it all gets, especially in light of the fact that there are so many points that can serve as a ‘hop’ or a ‘coupling’ point!

So… Well… Nothing. That’s it! I am done! I realize this has been another long and difficult story, but I hope you appreciated and that it shed some light on what’sĀ reallyĀ behind those simplified stories of what quantum mechanics is all about. It’s all weird and, admittedly, not so easy to understand, but I wouldn’t say an understanding is really beyond the reach of us, common mortals. šŸ™‚

Post scriptum: When you’ve reached here, you may wonder: so where’s the final formula then for E(A to B)? Well… I have no easy formula for you. From what I wrote above, it should be obvious that we’re talking some really awful-looking integral and, because it’s so awful, I’ll let you find it yourself. šŸ™‚

I should also note another reason why I am reluctant to identify n with m. The formulas in Feynman’s QED are definitelyĀ notĀ the standard ones. The more standard formulations will use theĀ gauge coupling parameterĀ about which I talked already. I sort of discussed it, indirectly, in my first comments on Feynman’s QED, when I criticized some other part of the book, notably its explanation of the phenomenon of diffraction of light, which basically boiled down to:Ā ā€œWhen you try to squeeze light too much [by forcing it to go through a small hole], it refuses to cooperate and begins to spread outā€, because “there are not enough arrows representing alternative paths.”

NowĀ thatĀ raises a lot of questions, and very sensible ones, because that simplification is nonsensical.Ā Not enough arrows?Ā That statement doesn’t make sense. We can subdivide space in as many paths as we want, and probability amplitudes don’t take up any physical space. We can cut up space in smaller and smaller pieces (so we analyze more paths within the same space). The consequence – in terms of arrows – is that directions of our arrows won’t change but their length will be much and much smaller as we’re analyzing many more paths. That’s because of the normalization constraint. However, when adding them all up – a lot of very tiny ones, or a smaller bunch of bigger ones – we’ll still get the same ‘final’ arrow. That’s because the direction of those arrows depends on theĀ lengthĀ of the path, and the length of the path doesn’t change simply because we suddenly decide to use some other ‘gauge’.

Indeed, theĀ real question is: what’s a ā€˜small’ hole? What’s ā€˜small’ and what’s ā€˜large’ in quantum electrodynamics? Now, I gave an intuitive answer to that question in that post of mine, but it’s much more accurate than Feynman’s, or Leighton’s. The answer to that question is: there’s some kind of natural ‘gauge’, and it’s related to the wavelength. So the wavelength of a photon, or an electron, in this case, comes with some kind of scale indeed. That’s why the fine-structure constant is often written in yet another form:

α = 2Ļ€re/Ī»e = rekeĀ 

Ī»e and keĀ are the Compton wavelength and wavenumber of the electron (soĀ keĀ is notĀ the Coulomb constant here). The Compton wavelength is the de Broglie wavelength of the electron. [You’ll find that Wikipedia defines it as “the wavelength that’sĀ equivalent to the wavelength of a photon whose energy is the same as the rest-mass energy of the electron”, but that’s a very confusing definition, I think.]

The point to note is that theĀ spatialĀ dimension in both the analysis of photons as well as of matter waves, especially in regard to studying diffraction and/or interference phenomena, is related to the frequencies, wavelengths and/or wavenumbers of the wavefunctions involved. There’s a certain ‘gauge’ involved indeed, i.e.Ā some measure that is relative, like the gauge pressure illustrated below. So that’s where thatĀ gauge parameterĀ g comes in. And the fact that it’s yet another number that’s closely related to that fine-structure constant is… Well… Again… That alpha number is a very magic number indeed… šŸ™‚

abs-gauge-press

Post scriptumĀ (5 October 2015):

Much stuff is physics is quite ‘magical’, but it’s never ‘too magical’. I mean: there’s always an explanation. So there is a very logical explanation for the above-mentioned deep connection between the charge of an electron, its energy and/or mass, its various radii (or physical dimensions) and the coupling constant too. I wrote a piece about that, much later than when I wrote the piece above. I would recommend you read that piece too. It’s a piece in which I do take the magic out of ‘God’s number’. Understanding it involves a deep understanding of electromagnetism, however, and that requires some effort. It’s surely worth the effort, though.