Sycobob
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Homework Statement
From Sean Carroll's notes on general relativity (chapter 1, pg. 20):
Show that F_{[\alpha\beta,\gamma]} = 0 is equivalent to half of the Maxwell equations.
Homework Equations
F_{\mu\nu} is the electromagnetic tensor
\Phi_{,\nu} \equiv \partial_{\nu}\Phi
F_{i0}= E_{i}
F_{ij}= \epsilon^{ijk}B_{k}
The Attempt at a Solution
I'm specifically looking to turn Maxwell's (homogeneous) equations into tensor form, not just show that they fall out of F_{[\alpha\beta,\gamma]} = 0. I sort of have a solution, but I feel like I'm missing a step.
<br /> \begin{eqnarray*}<br /> \nabla×\textbf{E} + \partial_{t}\textbf{B} = 0 \\<br /> \nabla\cdot \textbf{B} = 0<br /> \\<br /> \\<br /> \epsilon^{ijk}\partial_{j}E_{k} + \partial_{0}B^{i} = 0 \\<br /> \partial_{i}B^{i} = 0<br /> \\<br /> \\<br /> \epsilon^{ijk}\partial_{j}F_{k0} + \frac{1}{2}\epsilon^{ijk}\partial_{0}F_{jk} = 0 \\<br /> \frac{1}{2}\epsilon^{ijk}\partial_{i}F_{jk} = 0<br /> \end{eqnarray*}<br />
which can be rewritten as:
\epsilon^{\mu\nu\rho\sigma}\partial_{\rho}F_{\mu \nu} = 0
which, up to a normalization constant, is just:
F_{[\alpha\beta,\gamma]} = 0
My question is about going from step 3 to step 4. I sort of pulled it out of my hat and checked that it was correct (term by term). I'm looking for some kind of justification for this step, or a nudge in the right direction if I'm approaching this all wrong.
Also, I'm still getting the hang of tensor notation, and I feel like equation 4 doesn't make sense. Only 3 indices are contracted, leaving the right side a vector, not a scalar. On the other hand, trying to use the Levi-Civita tensor with 3 indices here seems wrong too, as the indices run from 0 to 4 leaving you with stuff like \epsilon^{013}.