Global GR Theorems without Energy Conditions?

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SUMMARY

The discussion centers on the limitations of traditional energy conditions (weak, null, dominant) applied to the stress-energy tensor in proving global results such as the singularity theorem and the positive energy theorem. Participants highlight the need for re-evaluating these theorems using plausible constraints on the matter Lagrangian instead of relying solely on energy conditions. A referenced paper (http://arxiv.org/abs/1012.6038) explores the implications of scalar fields on energy conditions, indicating that certain scenarios, including those involving a nonzero cosmological constant, challenge previous conclusions drawn from cosmic microwave background (CMB) observations.

PREREQUISITES
  • Understanding of energy conditions in general relativity
  • Familiarity with the stress-energy tensor
  • Knowledge of the Lagrangian formulation in physics
  • Basic concepts of cosmology and cosmic microwave background (CMB) analysis
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  • Research the implications of scalar fields on energy conditions in general relativity
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  • Examine the effects of a nonzero cosmological constant on general relativity theorems
  • Explore recent papers addressing the limitations of traditional energy conditions in theoretical physics
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The discussion is beneficial for theoretical physicists, cosmologists, and researchers interested in the foundations of general relativity and the implications of energy conditions on global theorems.

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It has come up a few times in recent threads here that the energy conditions on the stress-energy tensor (weak, null, dominant, etc) traditionally used to prove global results (e.g. the singularity theorem, the positive energy theorem, geodesic motion theorems*) are problematic: they allow more than they should, yet prohibit physically plausible scenarios as well. It strikes me that the original motivation for these was the sense of 'generality' - the you don't need to assume a theory of matter. However, since this has not panned out so well, I ask:

Does anyone know of attempts to re-prove such theorems on the basis of plausible constraints on the matter Lagrangian (or general forms of the Lagrangian) rather than the traditional energy conditions?



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*There are papers proving rigorously that if you carefully take the limit as a body shrinks in size and mass, that it must follow a geodesic of the background geometry. Such theorems as I've seen must assume an energy condition as part of the proof. I have also seen a paper that shows that the energy conditions is *necessary*. That is, if you do the limiting process without any constraint on T, not only is non-geodesic motion possible, but even spacelike paths are possible. This is not really surprising given the possible properties of exotic matter.
 
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I found a paper on this theme:

http://arxiv.org/abs/1012.6038

This specifically addresses the issue of scalar fields which are a thorn in the side of the energy conditions.
 
I think there are some cases where you can't re-prove the theorems because there are known counterexamples. For instance, the nonzero cosmological constant violates some energy conditions, and I think this means that certain inferences made in the past from CMB observations have had to be reanalyzed.
 

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