Rewriting Maxwell's Equations in Tensor Form

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SUMMARY

The discussion focuses on rewriting Maxwell's equations in tensor form, specifically addressing the equivalence of the condition F_{[\alpha\beta,\gamma]} = 0 to half of Maxwell's equations. Participants explore the transformation of the homogeneous equations into tensor notation, highlighting the electromagnetic tensor F_{\mu\nu} and its components. Key equations include the use of the Levi-Civita symbol and the implications of index contraction in tensor calculus. The conversation emphasizes the need for clarity in tensor notation and the correct application of mathematical identities.

PREREQUISITES
  • Understanding of tensor calculus and notation
  • Familiarity with Maxwell's equations and their physical significance
  • Knowledge of the Levi-Civita symbol and its properties
  • Basic concepts of differential geometry as applied to physics
NEXT STEPS
  • Study the properties of the Levi-Civita symbol in tensor calculus
  • Learn about the contraction of tensors and its implications in physics
  • Explore the derivation of Maxwell's equations from first principles in tensor form
  • Investigate the relationship between forms and their independent components in various dimensions
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Physicists, mathematicians, and students studying general relativity or electromagnetism who seek to deepen their understanding of tensor analysis and its application to Maxwell's equations.

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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}.
 
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The first equation in your step 3 is actually three equations, one for each value of i. And the second equation is just one. That's why the final result is a set of four equations.

I think the final step will be easier to understand if you make sure that you understand every step of the following rewrites: (Here A is anything with three indices from 0 to 3).

\begin{align}
&\varepsilon^{ijk} A_{ijk} =\varepsilon^{ijk0} A_{ijk} =\varepsilon^{\mu\nu\rho 0} A_{\mu\nu\rho}\\
&\varepsilon^{ijk} A_{0jk} =\varepsilon^{0jki} A_{0jk} =\varepsilon^{0\nu\rho i} A_{0\nu\rho} =\varepsilon^{\mu\nu\rho i} A_{\mu\nu\rho}
\end{align}
 
Fredrik said:
The first equation in your step 3 is actually three equations, one for each value of i. And the second equation is just one. That's why the final result is a set of four equations.

I think the final step will be easier to understand if you make sure that you understand every step of the following rewrites: (Here A is anything with three indices from 0 to 3).

\begin{align}
&\varepsilon^{ijk} A_{ijk} =\varepsilon^{ijk0} A_{ijk} =\varepsilon^{\mu\nu\rho 0} A_{\mu\nu\rho}\\
&\varepsilon^{ijk} A_{0jk} =\varepsilon^{0jki} A_{0jk} =\varepsilon^{0\nu\rho i} A_{0\nu\rho} =\varepsilon^{\mu\nu\rho i} A_{\mu\nu\rho}
\end{align}
need help here

how did you obtain these rules>
thank you
 
How many independent components does a 1-form have in 4 dimensions? And a 3-form? This is a first step to check whether your result makes sense (hint: it does :P )

Hit your equation then with an (4-comp.) epsilon symbol with the free index contracted. Find/derive the identities of contracted epsilon symbols in terms of kronecker deltas and apply those.

Hope this helps ;)
 
haushofer said:
How many independent components does a 1-form have in 4 dimensions? And a 3-form? This is a first step to check whether your result makes sense (hint: it does :P )

Hit your equation then with an (4-comp.) epsilon symbol with the free index contracted. Find/derive the identities of contracted epsilon symbols in terms of kronecker deltas and apply those.

Hope this helps ;)
thank for your help
i have trouble in "εijk A0jk=ε0jki A0jk "
i get stuck in this equation
i don't know how can they put a zero into the εijk
such that εijk ---> ε0jki
i think A0 is "fixed variable" and you cannot do anything for it
right? if you put a zero there,then A0 will become dummy variable (so we can contract an upper and lower index together)
 

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