Raising indices in curved space

bdforbes
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In curved space, can I raise an index on a tensor that is being differentiated? Ie, is the following true?

g^{\mu\lambda}\partial^\nu(F_{\mu\nu})=\partial^\nu(F^\lambda_\nu)
 
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Only if the metric tensor is independent of x_{\nu}.
 
This is troubling. I'm trying to obtain Maxwell's Equations from the Lagrangian, and since we have indices both up and down ie F^{\mu\nu}F_{\mu\nu}, varying with respect to \delta A_\lambda inevitably introduces metrics:

\delta F^{\mu\nu}=\partial^\mu g^{\nu\lambda}\delta A_\lambda - \partial^\nu g^{\mu\lambda}\delta A_\lambda

Integrating a term:

\int d^4x\sqrt{-g}(\delta F^{\mu\nu} \delta F_{\mu\nu})
= \int d^4x\sqrt{-g}\left[\partial^\mu(g^{\nu\lambda}\delta A_\lambda)F_{\mu\nu} - \partial^\nu(g^{\mu\lambda}\delta A_\lambda)F_{\mu\nu}\right]
= \int d^4x\sqrt{-g}(g^{\mu\lambda} \partial^\nu F_{\mu\nu} - g^{\nu\lambda} \partial^\mu F_{\mu\nu})\delta A_\lambda

And now I have these terms which are confusing me.
 
What happens if you vary

g_{\mu b}g_{\nu a}F^{ab}F^{\mu\nu}

instead ?
 
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I will try that, but I suspect it is equivalent.
If I had used covariant derivatives the whole time, there would be no problem. But here
http://en.wikipedia.org/wiki/Maxwell's_equations_in_curved_spacetime#Summary
it states that the extra terms introduced by using covariant derivatives would cancel out. So maybe my original method is fine.
Of course, I was stupid to overlook look this fact:
\delta F^{\mu\nu} F_{\mu\nu}=\delta F_{\mu\nu} F^{\mu\nu}
 
This may interest you.

"Maxwell’s Equations In a Gravitational Field" by Andrew E. Blechman
 

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