Phase invariance of an EM wave in special relativity

quasar_4
Messages
273
Reaction score
0

Homework Statement



So I'm trying to show for a specific, given EM plane wave in vacuum that

kx - \omega t = k' x' - \omega' t'

but I'm running into some difficulties. I'm hoping someone can show me where I'm going wrong. Here's the setup:

In the lab frame K, a plane EM wave traveling in vacuum has an electric field given by

\vec{E}(\vec{x},t) = \hat{z} E0 \cos{(\frac{k}{\sqrt{2}} (x+y) - \omega t)}

where E0, k are positive real constants, omega = ck

Homework Equations



Maxwell's equations
Lorentz transformation

The Attempt at a Solution



First I found the B field in K using Faraday's law. Then I used the standard transformations in Jackson to go from E, B to E', B' in the K' frame.

My electric field in the K' frame is

\vec{E'}(\vec{x},t) =\hat{z} \gamma (1-\beta) \cos{(\frac{k}{\sqrt{2}} (x+y)-\omega t)}

Now I want to use the Lorentz transformation,

x = \gamma (x' + \beta c t') \text{ , } ct = \gamma (c t' + \beta x')

to put E' in terms of the primed coordinates. If I understand Jackson correctly (he says phase of a plane wave is an invariant), then shouldn't we be able to demand that

\frac{k}{\sqrt{2}} (x+y) -\omega t = \frac{k'}{\sqrt{2}} (x'+y') -\omega' t'

?

I'm trying to prove this, doing simple substitution with x, y, t -> x', y', t', but I can't get the factors of k' and w' to come out correctly because of the square root of 2. I'm stuck at:
\frac{k}{\sqrt{2}} (x+y) -\omega t = \gamma \left[k x' (\frac{1}{\sqrt{2}}-\beta) + \omega t' (\frac{\beta}{\sqrt{2}}-1) \right] + \frac{y' k}{\sqrt{2}}

I don't know my initial assumption is wrong, or the algebra is just tricky. Any help appreciated!
 
Physics news on Phys.org
quasar_4 said:
If I understand Jackson correctly (he says phase of a plane wave is an invariant), then shouldn't we be able to demand that

\frac{k}{\sqrt{2}} (x+y) -\omega t = \frac{k'}{\sqrt{2}} (x'+y') -\omega' t'

?
No, when he says the phase is invariant, he means

k_\mu x^\mu = k'_\mu x'^\mu

where k'^\mu = \Lambda^\mu_\nu k^\nu. Though the x and y components of k are equal in frame K, they generally won't be in K'.
 
Ok, thanks.
 
##|\Psi|^2=\frac{1}{\sqrt{\pi b^2}}\exp(\frac{-(x-x_0)^2}{b^2}).## ##\braket{x}=\frac{1}{\sqrt{\pi b^2}}\int_{-\infty}^{\infty}dx\,x\exp(-\frac{(x-x_0)^2}{b^2}).## ##y=x-x_0 \quad x=y+x_0 \quad dy=dx.## The boundaries remain infinite, I believe. ##\frac{1}{\sqrt{\pi b^2}}\int_{-\infty}^{\infty}dy(y+x_0)\exp(\frac{-y^2}{b^2}).## ##\frac{2}{\sqrt{\pi b^2}}\int_0^{\infty}dy\,y\exp(\frac{-y^2}{b^2})+\frac{2x_0}{\sqrt{\pi b^2}}\int_0^{\infty}dy\,\exp(-\frac{y^2}{b^2}).## I then resolved the two...
Hello everyone, I’m considering a point charge q that oscillates harmonically about the origin along the z-axis, e.g. $$z_{q}(t)= A\sin(wt)$$ In a strongly simplified / quasi-instantaneous approximation I ignore retardation and take the electric field at the position ##r=(x,y,z)## simply to be the “Coulomb field at the charge’s instantaneous position”: $$E(r,t)=\frac{q}{4\pi\varepsilon_{0}}\frac{r-r_{q}(t)}{||r-r_{q}(t)||^{3}}$$ with $$r_{q}(t)=(0,0,z_{q}(t))$$ (I’m aware this isn’t...
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
Back
Top