Commutator notation in classical field theory

paco_uk
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Homework Statement



Could someone please explain what is meant by the term:

\partial_{[ \mu}F_{\nu \rho ]}

Homework Equations



I have come across this in the context of Maxwells equations where F^{\mu \nu} is the field strength tensor and apparently:

\partial_{[ \mu}F_{\nu \rho ]} =0

follows "trivially" from

F_{\mu \nu} = \partial_{\mu} A_{\nu} - \partial_{\nu} A_{\mu}



The Attempt at a Solution



I don't understand what the notation means and I haven't found it defined anywhere. Do all three indices get permuted somehow?
 
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Would you please fix your latex tags?
They should be [ tex ]...[ /tex ] (that is: forward slash, but no spaces within the tag).

You'll see that your equation will look "strange" then.
Could you perhaps fix that as well?
 
Sorry about the mess. I've cleared up the latex tags. What's there now does indeed look strange to me but is what is written in the lecture notes. I don't know what the commutator bracket round the subscripts means.
 
paco_uk said:
I don't understand what the notation means and I haven't found it defined anywhere. Do all three indices get permuted somehow?

Yes. This is the antisymmetrizing operation. A good explanation is given in Prof. Maloney's notes and lecture recordings. It's also found in many good reference books on GR and differential geometry.

http://www.physics.mcgill.ca/~maloney/514/

Here is a PDF of the relevant lecture notes, but it's helpful to listen to the lectures if you have time.
 

Attachments

The notation makes sense, if you learn about differential forms on the space-time manifold. The F is then a 2-form, and dF =0 is a consequence of the 2-nd degree nilpotency of the exterior differential.
 
Thanks very much. I've never done a course on General Relativity so I'm pretty shaky on all this. I look forward to listening to the lectures.
 
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