Klein Gordon Invariance in General Relativity

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SUMMARY

The discussion centers on the invariance of the Klein-Gordon Lagrangian under linear diffeomorphisms in curved spacetime. The Lagrangian is expressed as $$L=\sqrt{-g}\left(g^{\mu\nu}\partial_\mu \phi \partial_\nu \phi-\frac{m^2}{2}\phi^2\right)$$. Participants clarify that the invariance is not straightforward due to the presence of the volume element $$\sqrt{-g}$$ and emphasize that the action must be treated as a scalar density for the field equations to remain covariant. The Lie derivative's role in this context is also highlighted, indicating that the transformation of the metric does not yield a zero result.

PREREQUISITES
  • Understanding of the Klein-Gordon equation and its formulation in curved spacetime.
  • Familiarity with the concept of diffeomorphisms and their implications in general relativity.
  • Knowledge of scalar densities and their transformation properties under coordinate changes.
  • Basic grasp of action principles in field theory and their relation to covariant equations of motion.
NEXT STEPS
  • Study the properties of the Lie derivative in the context of general relativity.
  • Explore the concept of scalar densities and their role in field theories.
  • Investigate the relationship between gauge invariance and diffeomorphism invariance in field theories.
  • Review the action principle and its application in deriving covariant field equations.
USEFUL FOR

This discussion is beneficial for theoretical physicists, particularly those specializing in quantum field theory in curved spacetime, as well as graduate students seeking to deepen their understanding of the Klein-Gordon Lagrangian and its invariance properties.

phyz2
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Confused bout KG Lagrangian in curved space
Hello!
I'm starting to study curved QFT and am slightly confused about the invariance of the Klein Gordon Lagrangian under a linear diffeomorphism.
This is $$L=\sqrt{-g}\left(g^{\mu\nu}\partial_\mu \phi \partial_\nu \phi-\frac{m^2}{2}\phi^2\right),$$
I don't see how ##g^{\mu\nu}\to g^{\mu\nu}+\partial^{(\mu}\xi^{\nu)}## should leave this invariant.. I get and extra piece which is ##\sqrt{-g} \partial^{(\mu}\xi^{\nu)} \partial_\mu \phi \partial_\nu \phi## and I don't see how this should be zero, even at the linear level.

Thanks for any help!
 
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What you wrote down as ##L## is not invariant because it includes the ##\sqrt g## from the volume element.

The expression in the parenthesis is manifestly a scalar.
 
Orodruin said:
The expression in the parenthesis is manifestly a scalar.
For this to be true in curved spacetime (which is what I understand the OP to be asking about), wouldn't the derivatives need to be covariant derivatives instead of partial derivatives?
 
PeterDonis said:
For this to be true in curved spacetime (which is what I understand the OP to be asking about), wouldn't the derivatives need to be covariant derivatives instead of partial derivatives?
For (first) derivatives of scalars there is no difference.
 
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One should emphasize that ##\sqrt{-g}\mathrm{d}^4 x## is generallt invariant too. So the action is generally invariant and thus the resulting field equations too. That makes the action principle so useful for finding adequate equations, that are covariant under a given symmetr.
 
Agreed, I considered it subtextual that the volume element is invariant but I could have been more specific for clarity.
 
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phyz2 said:
Summary:: Confused bout KG Lagrangian in curved space

Hello!
I'm starting to study curved QFT and am slightly confused about the invariance of the Klein Gordon Lagrangian under a linear diffeomorphism.
This is $$L=\sqrt{-g}\left(g^{\mu\nu}\partial_\mu \phi \partial_\nu \phi-\frac{m^2}{2}\phi^2\right),$$
I don't see how ##g^{\mu\nu}\to g^{\mu\nu}+\partial^{(\mu}\xi^{\nu)}## should leave this invariant.. I get and extra piece which is ##\sqrt{-g} \partial^{(\mu}\xi^{\nu)} \partial_\mu \phi \partial_\nu \phi## and I don't see how this should be zero, even at the linear level.

Thanks for any help!
The transformation for the metric you give is (a linearization of) the Lie derivative, an "active diffeomorphism". The Lie derivative of the Lagrangian is not zero.
 
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haushofer said:
The transformation for the metric you give is (a linearization of) the Lie derivative, an "active diffeomorphism". The Lie derivative of the Lagrangian is not zero.
Thanks! Could you elaborate a bit more? I thought the invariance under diffeos would be equivalent to the gauge invariance of the, say, Maxwell Lagrangian.. in that case the change of the action is zero.
 
The key is the action. If the action is invariant under general coordinate transformations then for sure the field-equations of motion derived from it are covariant equations. That implies that the Lagrangian ##\mathfrak{L}## should be a scalar density (!) or you write ##\mathfrak{L}=\sqrt{-g} L##, where ##L## is a scalar. Then
$$A=\int \mathrm{d}^4 q \mathfrak{L} = \int \mathrm{d}^4 q \sqrt{-g} L$$
is a scalar and thus the field equations of motion derived from Hamilton's principle using this action are generally covariant.
 
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phyz2 said:
Thanks! Could you elaborate a bit more? I thought the invariance under diffeos would be equivalent to the gauge invariance of the, say, Maxwell Lagrangian.. in that case the change of the action is zero.
Sorry for the late reply. I understand your confusion. Let's take a scalar. Under a g.c.t. one has that phi(x) = phi'(x'). But the Lie derivative, what's commonly called an "infinitesimal g.c.t.", compares phi'(x) and phi(x) instead of phi'(x') and phi(x). Watch those primes like a hawk! And the Lie derivative of a scalar is in general non-zero, of course.

The Lagrangean density is a scalar density, so you should consider how such a density transforms under "infinitesimal g.c.t.'s". It's been a while, but with proper boundary conditions you should get a total derivative such that the action functional is invariant. See e.g. d'Inverno.
 
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  • #11
vanhees71 said:
The key is the action. If the action is invariant under general coordinate transformations then for sure the field-equations of motion derived from it are covariant equations. That implies that the Lagrangian ##\mathfrak{L}## should be a scalar density (!) or you write ##\mathfrak{L}=\sqrt{-g} L##, where ##L## is a scalar. Then
$$A=\int \mathrm{d}^4 q \mathfrak{L} = \int \mathrm{d}^4 q \sqrt{-g} L$$
is a scalar and thus the field equations of motion derived from Hamilton's principle using this action are generally covariant.
Yes, but that's not the issue as I understand it.
 

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