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™‚

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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:

at2 – ax2 – ay2 – az2 = 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 – Ax2 – Ay2 – Az2 = 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.

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