Gravitational Wave Local Energy: Not Gauge Invariant?

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SUMMARY

The discussion centers on the gauge invariance of the stress-energy tensor for linearized gravitational fields as defined by Wald. It is established that this tensor is not gauge invariant due to the use of the flat metric η instead of the full metric, which leads to complications in transformations between metrics. The participants emphasize that while tensors change with coordinate transformations, they retain specific properties, such as the inability to convert a zero tensor into a non-zero tensor. The conversation also references Carroll's work, highlighting the importance of averaging over regions of space to obtain meaningful results and the necessity of gauge invariance in energy calculations.

PREREQUISITES
  • Understanding of linearized gravitational fields
  • Familiarity with stress-energy tensors in general relativity
  • Knowledge of gauge transformations in physics
  • Basic concepts of tensor calculus
NEXT STEPS
  • Study Wald's "General Relativity" for a deeper understanding of stress-energy tensors
  • Examine Carroll's discussions on gauge invariance in "Spacetime and Geometry"
  • Research the implications of averaging in gravitational wave physics
  • Explore the relationship between coordinate transformations and tensor properties
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Physicists, graduate students in general relativity, and researchers focusing on gravitational wave physics and gauge invariance issues.

alemsalem
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I'm reading wald page 85, and he defines a stress-energy tensor for the linearized gravitational field. he mentions that it not gauge invariant as a problem. but isn't that a general property of any tensor (except scalars). so any stress-energy tensor will not be gauge invariant (change of coordinates).
is it because we're using η and not the full metric?
 
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When you're dealing with the linearized approximation, you have two metrics: the flat pace metric and the curved space metric. In this context, a gauge transformation refers to a transformation that alters the relationship between the two. In infinitesimal form, hμν → hμν + ξμ,ν + ξν,μ.
 
If you think it might be helpful to get a different presentation of the same thing, Carroll has a discussion on p. 162: http://arxiv.org/abs/gr-qc/?9712019

Although it's true that any tensor changes with a change of coordinates (in the sense that its representation in those coordinates is different), tensors do have a couple of important properties: (1) a change of coordinates never changes a zero tensor to a nonzero tensor, and (2) you can form scalars by contracting indices on tensors.

I think what Wald and Carroll have in mind as being objectionable about the stress-energy "tensor" t amounts to saying that it fails to have these properties.

You typically only get meaningful results from t by averaging over a region of space that is large compared to a wavelength, and the failure of #1 clearly shows what could go wrong if you didn't. As a non-fancy way of discussing this, just imagine trying to calculate the local energy density of a gravitational wave from the square of the ordinary gravitational field vector g from freshman physics. We know this can't be right, by the equivalence principle, since we can always make g=0 at any given spacetime location by going into a free-falling frame.

As an example of why #2 is important, see Carroll's discussion on p. 169. To get the total energy radiated to infinity, he has to form something that isn't a scalar according to the grammar of index gymnastics, and then a separate calculation is required in order to show that this thing really is gauge-invariant.
 

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