I Deviations of conservation laws in cosmological evolution?

AI Thread Summary
In General Relativity, energy conservation is maintained locally, meaning energy cannot be created or destroyed in local processes, despite the challenges of defining global energy in an expanding universe. Observations of large-scale structures, such as galaxy clusters, show no deviations from strict conservation laws, as local energy conservation holds true. The concept of energy "not being conserved" in GR refers to the absence of a well-defined global energy in curved spacetimes, not to the possibility of perpetual motion or free energy. The effects of tidal forces from spacetime expansion are acknowledged but do not indicate violations of energy conservation. Overall, the principles of energy conservation remain intact within the framework of General Relativity.
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Deviations of conservation laws in the context of cosmological evolution?
If energy is "not conserved" in General Relativity (or at least, it is difficult to define it) in the context of an expanding accelerating spacetime (like it happens in our Universe), are there any observations of deviations from the strict conservation laws in the evolution and formation of large scale structures (like clusters or superclusters of galaxies for instance)?

For example, in some articles about the study of galaxies and clusters evolutions and formations, sometimes the effects of the "tidal force" from spacetime expansion is considered... Has the expansion changed the energy or momentum of these systems somehow?
 
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Suekdccia said:
If energy is "not conserved" in General Relativity
This doesn't mean what it seems to mean.

When you think of "energy conservation", you're probably thinking of local energy conservation: roughly speaking, that energy can't be created or destroyed in any local process. That is still true in GR; its mathematical expression is that the covariant divergence of the stress-energy tensor is zero.

What "energy is not conserved" in GR actually means is that, except for certain special cases (of which our expanding universe is not one), there is no well-defined global energy that is conserved. But that doesn't mean you can make a perpetual motion machine or get free energy from nothing. All it means is that general curved spacetimes don't have a certain mathematical property that many physicists think it would be "nice" to have.

Suekdccia said:
are there any observations of deviations from the strict conservation laws in the evolution and formation of large scale structures (like clusters or superclusters of galaxies for instance)?
No. These are all local processes and, as above, local energy conservation holds in GR. For example, the energy radiated away as a bound system (say a star) forms is exactly equal to the decrease in the externally measured mass of the system.

Suekdccia said:
in some articles about the study of galaxies and clusters evolutions and formations, sometimes the effects of the "tidal force" from spacetime expansion is considered
Can you give a reference?
 
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