Gravitational Wave Local Energy: Not Gauge Invariant?

In summary, the stress-energy tensor for the linearized gravitational field is not gauge invariant, which is a general property of tensors. This is due to the use of the flat space metric instead of the full metric in the linearized approximation. This leads to potential issues with calculating energy density and total energy radiated.
  • #1
alemsalem
175
5
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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  • #2
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.
 
  • #3
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.
 

Related to Gravitational Wave Local Energy: Not Gauge Invariant?

1. What are gravitational waves?

Gravitational waves are ripples in the fabric of space-time caused by the acceleration of massive objects, such as black holes or neutron stars. They were predicted by Einstein's theory of general relativity and were first observed in 2015.

2. How is gravitational wave local energy calculated?

Gravitational wave local energy is calculated using the energy-momentum tensor, which describes the distribution of energy and momentum in space-time. The energy density of gravitational waves is typically very small, making it a challenging measurement to make.

3. Why is gravitational wave local energy not gauge invariant?

Gauge invariance is a mathematical concept that means the equations describing a physical system are independent of the choice of coordinates used. Gravitational wave local energy is not gauge invariant because it depends on the coordinate system used to measure it, and different coordinate systems can give different values.

4. How do scientists detect gravitational waves?

Scientists use a variety of instruments, such as the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the European Gravitational Observatory (EGO), to detect gravitational waves. These instruments use lasers and mirrors to measure tiny distortions in space-time caused by passing gravitational waves.

5. What are the potential applications of studying gravitational wave local energy?

Studying gravitational wave local energy can help us understand the nature of gravity and the behavior of massive objects in the universe. It can also provide insights into the properties of the early universe and help us develop new technologies for detecting and manipulating gravitational waves.

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