Undergrad Deriving E&B Fields from Plane Wave 4-Potential

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SUMMARY

This discussion focuses on deriving the electric and magnetic fields from the four-potential ##\mathbf{A} = (A^t , \mathbf{a})## in the Lorenz gauge for a plane wave. The magnetic field is derived as ##\mathbf{B} = \sin (\mathbf{K} \cdot \mathbf{R}) (\mathbf{k} \times \mathbf{c})##, while the electric field is expressed as ##\mathbf{E} = \sin (\mathbf{K} \cdot \mathbf{R}) \left( C^t \mathbf{k} + k \mathbf{c} \right)##. The discussion raises questions about the conditions under which the components ##\mathbf{c}## and ##\mathbf{k}## are perpendicular in all Lorentz frames and the implications of sign conventions in the exponent of the plane wave. The importance of verifying the Lorentz invariance of these relationships is emphasized.

PREREQUISITES
  • Understanding of four-potential in electromagnetism
  • Familiarity with Lorenz gauge conditions
  • Knowledge of vector calculus, particularly curl operations
  • Concept of Lorentz invariance in special relativity
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  • Study the derivation of electromagnetic fields from four-potential in detail
  • Explore the implications of Lorentz invariance on vector components
  • Investigate different sign conventions in Minkowski space and their effects on wave equations
  • Learn about the physical significance of polarization vectors in electromagnetic waves
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Physicists, particularly those specializing in electromagnetism and special relativity, as well as graduate students studying wave phenomena and field theory.

SiennaTheGr8
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TL;DR
Having trouble deriving the electric field of a plane wave from the four-potential.
I'm trying to derive the electric and magnetic fields of a plane wave from the four-potential ##\mathbf{A} = (A^t , \mathbf{a}) ## in the Lorenz gauge. Given:

##\mathbf{A}(\mathbf{R}) = \Re \left( \mathbf{C} e^{i \mathbf{K} \cdot \mathbf{R}} \right)##

for constant future-pointing lightlike ##\mathbf{K} = (K^t, \mathbf{k})## and constant ##\mathbf{C} = (C^t , \mathbf{c})## orthogonal to ##\mathbf{K}##, I think I correctly get the magnetic field by taking the real part of this:

##\nabla \times \mathbf{a} = \nabla \times \left( \mathbf{c} e^{i \mathbf{K} \cdot \mathbf{R}} \right) = \nabla e^{i \mathbf{K} \cdot \mathbf{R}} \times \mathbf{c}##,

which gives me ##\mathbf{B} = \sin (\mathbf{K} \cdot \mathbf{R}) (\mathbf{k} \times \mathbf{c}) ##. That seems reasonable, and if it's right then I expect ##\mathbf{E}## to have magnitude ##\sin (\mathbf{K} \cdot \mathbf{R}) \Vert \mathbf{k} \times \mathbf{c} \Vert## and be perpendicular to both ##\mathbf{B}## and ##\mathbf{k}## (and perhaps parallel to ##\mathbf{c}##?). But I'm having trouble:

##- \nabla A^t - \partial^t \mathbf{a} = - \nabla \left( C^t e^{i \mathbf{K} \cdot \mathbf{R}} \right) - \partial^t \left( \mathbf{c} e^{i \mathbf{K} \cdot \mathbf{R}} \right) = -C^t \nabla e^{i \mathbf{K} \cdot \mathbf{R}} - \mathbf{c} \partial^t e^{i \mathbf{K} \cdot \mathbf{R}}##.

If the first term vanishes, taking the real part of the second term I get ##\mathbf{E} = \sin (\mathbf{K} \cdot \mathbf{R}) k \mathbf{c}##, which works if it's true that ##\mathbf{c} \parallel \mathbf{E}## (correct magnitude, and correct right-handed set for ##\mathbf{E}##, ##\mathbf{B}##, and ##\mathbf{k}##). Otherwise, for the first term I get:

##-C^t \nabla e^{i \mathbf{K} \cdot \mathbf{R}} = -i e^{i \mathbf{K} \cdot \mathbf{R}} C^t \mathbf{k}##,

whose real part I think is ##\sin (\mathbf{K} \cdot \mathbf{R}) C^t \mathbf{k}##, giving:

##\mathbf{E} = \sin (\mathbf{K} \cdot \mathbf{R}) \left( C^t \mathbf{k} + k \mathbf{c} \right) = \sin (\mathbf{K} \cdot \mathbf{R}) \left( (\mathbf{c} \cdot {\hat{\mathbf{k}}}) \mathbf{k} + k \mathbf{c} \right)##,

which doesn't seem right at all, unless it's true that ##\mathbf{c} \perp \mathbf{k}## in all frames (the condition under which the first term drops out). But I haven't been able to prove to myself that ##\mathbf{c} \perp \mathbf{k}## is a Lorentz-invariant statement. In fact, the notion seems silly, because unless I'm missing something it's equivalent to saying that I can't boost to a frame in which ##C^t \neq 0##.

Given that ##\mathbf{K}## is lightlike and ##\mathbf{C}## is orthogonal to it (and obviously spacelike), does it follow that their spatial three-vector components ##\mathbf{k}## and ##\mathbf{c}## are perpendicular in all Lorentz frames? If so, is it easily demonstrated? And if not, can you spot where I've gone off the rails?
 
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It occurs to me that I probably made a sign error (or errors), but that otherwise I was on the right track. If instead of:

## \mathbf{E} = \sin (\mathbf{K} \cdot \mathbf{R}) \left( C^t \mathbf{k} + K^t \mathbf{c} \right) ##

it were:

## \mathbf{E} = \sin (\mathbf{K} \cdot \mathbf{R}) \left( C^t \mathbf{k} - K^t \mathbf{c} \right) ##,

then ## \mathbf{E} \perp \mathbf{k}## as desired, since ##C^t \mathbf{k} \cdot \mathbf{k} - K^t \mathbf{c} \cdot \mathbf{k} = C^t K^{t \, 2} - C^t K^{t \, 2}## (and of course ##\mathbf{E} \perp \mathbf{B}##, since the former is coplanar with ##\mathbf{c}## and ##\mathbf{k}## while the latter is perpendicular to them).

Additionally, I think this sign correction gives ##E = B \propto ck \sin \theta_{[ \mathbf{c}, \mathbf{k} ]}##:

##\left( C^t \mathbf{k} - K^t \mathbf{c} \right) = ck \left( (\mathbf{\hat c} \cdot \mathbf{\hat k}) \mathbf{\hat k} - \mathbf{\hat c} \right) = ck \left( \mathbf{\hat k} \cos \theta - \mathbf{\hat c} \right)##,

where ##\Vert \mathbf{\hat k} \cos \theta - \mathbf{\hat c} \Vert ^2 = \left( \mathbf{\hat k} \cos \theta - \mathbf{\hat c} \right) \cdot \left( \mathbf{\hat k} \cos \theta - \mathbf{\hat c} \right) = 1 - \cos^2 \theta = \sin^2 \theta##.

I'll still have to find my sign error(s), but this looks promising (in case anyone was wondering...).
 
You can always choose your polarisation vector to have time-component of zero by subtracting from it a vector proportional to the wave vector. This will not change the EM fields.
 
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I have a related question—

In some sources I see a negative sign on the exponent like ##e^{-i \mathbf{K} \cdot \mathbf{R}}##, and in others I don't. Is this an arbitrary choice, or does it correspond to the chosen sign convention for the Minkowski dot product? That is, must one make the exponent negative if the Minkowski product gives ##K^t ct - \mathbf{k} \cdot \mathbf{r}##, so that the sinusoidal argument becomes ##\mathbf{k} \cdot \mathbf{r} - K^t ct##?
 
The real part of ##e^{-ik\cdot x}## and ##e^{ik\cdot x}## are the same. You will also get a redefinition of the polarisation vector. Of course, you will also get a difference in terms of the metric convention. Always check the metric convention.
 
Ah, I think I get it: cosine is obviously an even function, and although after differentiation (of the exponential) the real part will be an odd function (sine), you also inherit the correct sign from the exponent.

So it really is just a matter of preference whether to slap a negative sign up there (to get a classic "##x - t##" argument instead of "##t - x##"). Either way, you end up with a right-handed set of ##\mathbf{E}, \mathbf{B}, \mathbf{k}##, yeah?
 
In an inertial frame of reference (IFR), there are two fixed points, A and B, which share an entangled state $$ \frac{1}{\sqrt{2}}(|0>_A|1>_B+|1>_A|0>_B) $$ At point A, a measurement is made. The state then collapses to $$ |a>_A|b>_B, \{a,b\}=\{0,1\} $$ We assume that A has the state ##|a>_A## and B has ##|b>_B## simultaneously, i.e., when their synchronized clocks both read time T However, in other inertial frames, due to the relativity of simultaneity, the moment when B has ##|b>_B##...

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