What is the EM Lagrangian in curved spacetime?

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Discussion Overview

The discussion centers on the formulation of the electromagnetic (EM) Lagrangian in curved spacetime, particularly the differences between using covariant derivatives versus partial derivatives. Participants explore the implications of these choices on the invariance and correctness of the Lagrangian in the context of general relativity.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Exploratory

Main Points Raised

  • One participant presents the flat spacetime Lagrangian and proposes a curved spacetime generalization using covariant derivatives, questioning the validity of using partial derivatives as seen in some literature.
  • Another participant references Wald's work, which also employs covariant derivatives, suggesting a consensus on this approach among some sources.
  • There is a discussion about the invariance of equations under curvilinear coordinate transformations, with one participant noting that replacing partial derivatives with covariant derivatives would introduce extra terms that should cancel out due to the symmetry of the Christoffel symbols.
  • A participant expresses uncertainty about their own calculations regarding the cancellation of terms when substituting derivatives, indicating a need for further exploration.
  • Another participant introduces a more complex scenario involving manifolds with non-vanishing curvature and torsion, questioning how the field equations and Lagrangian would be formulated in such cases, suggesting that this remains an open area of inquiry.

Areas of Agreement / Disagreement

Participants do not reach a consensus on whether the use of partial or covariant derivatives is correct in the context of the EM Lagrangian in curved spacetime. Multiple competing views and uncertainties remain regarding the implications of these choices.

Contextual Notes

There are limitations related to the assumptions about the manifold, such as the presence of torsion and the compatibility of the affine connection with the metric, which are not fully resolved in the discussion.

pellman
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In flat space time the Lagrangian for the EM potential is (neglecting the source term)

[tex]\mathcal{L}_{flat}=-\frac{1}{16\pi}(\partial^{\mu}A^{\nu}-\partial^{\nu}A^{\mu})(\partial_{\mu}A_{\nu}-\partial_{\nu}A_{\mu})[/tex]

which is a scalar for flat spacetime. I would have expected the generalization to curved manifolds to be

[tex]\mathcal{L}_{curved}=-\frac{1}{16\pi}(\nabla^{\mu}A^{\nu}-\nabla^{\nu}A^{\mu})(\nabla_{\mu}A_{\nu}-\nabla_{\nu}A_{\mu})\sqrt{-g}[/tex]


However, the Wikipedia article for equations in curved spacetime[/url] gives the Lagrangian still in terms of the regular derivatives, not covariant derivatives. But [tex]\mathcal{L}_{flat}[/tex] is not a scalar in general, is it? I was just reading an article about covariance and Noether's theorem that likewise uses an EM Lagrangian in terms of partial derivatives instead of covariant derivatives.

So which is correct?

Edit: I just checked Gravitation (Misner, Thorne, Wheeler) and eq 22.19a gives the EM tensor as [tex]\nabla_{\mu}A_{\nu}-\nabla_{\nu}A_{\mu}[/tex]
 
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Wald also uses covariant derivatives on p. 455.

But did you see the following text in the WP article? "Despite the use of partial derivatives, these equations are invariant under arbitrary curvilinear coordinate transformations. Thus if one replaced the partial derivatives with covariant derivatives, the extra terms thereby introduced would cancel out."
 
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bcrowell said:
But did you see the following text in the WP article? "Despite the use of partial derivatives, these equations are invariant under arbitrary curvilinear coordinate transformations. Thus if one replaced the partial derivatives with covariant derivatives, the extra terms thereby introduced would cancel out."

No. I didn't read that . Thanks. I thought that might be it though and attempted to work it out myself earlier. I must have made a mistake. They didn't cancel for me. I'll give it another shot.
 
pellman said:
No. I didn't read that . Thanks. I thought that might be it though and attempted to work it out myself earlier. I must have made a mistake. They didn't cancel for me. I'll give it another shot.

They must cancel because of the symmetry of the Christoffel symbols.

[tex] A_{m;n} - A_{n;m} = A_{m,n}- A_{n,m} - {\Gamma^a}_{mn} A_a + {\Gamma^a}_{nm} A_a[/tex]
 
The title of the thread contains a good question. In the absence of torsion on the manifold (hypothesis which is of course not assumed in the question), the Lagrange density can contain partial derivatives, i/o covariant ones, because the necessary antisymmetry of the E-m field 2-form, coupled with the symmetry of the (probably metric compatible) connection would allow that.

A more interesting question arises though in the following case: Assuming the manifold has non-vanishing curvature and torsion and the affine connection is not metric compatible, what form would the field equations for the abelian gauge field have and moreover, assuming the existence of an action integral and a variational principle leading to the field equations, what form would the non-integrated Lagrangian have ??

I' m not aware of a full solution to my 2 queries, though I believe the first one has been already addressed (there's an article on arxiv.org as far as I recall).

Daniel
 
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