Advice on GR book specific to my needs

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SUMMARY

The discussion focuses on the practical applications of the stress-energy tensor in General Relativity (GR) after it is derived from a metric. Key areas of interest include cosmology topics such as brane worlds, brane gas cosmology, stability of compact extra dimensions, and the Casimir effect. Participants recommend checking the physical reasonableness of the stress-energy tensor by verifying energy conditions and using it to derive local energy and momentum densities through contraction with the observer's 4-velocity. Any standard GR textbook should cover these concepts adequately.

PREREQUISITES
  • Understanding of General Relativity principles
  • Familiarity with the stress-energy tensor and its significance
  • Knowledge of energy conditions in GR
  • Basic concepts of cosmology, particularly brane theory
NEXT STEPS
  • Research the energy conditions in General Relativity
  • Explore textbooks on General Relativity that cover the stress-energy tensor
  • Study the implications of brane gas cosmology in modern physics
  • Investigate the Casimir effect and its relevance in cosmological models
USEFUL FOR

Researchers and students in theoretical physics, particularly those focused on cosmology, General Relativity, and advanced topics like brane worlds and the Casimir effect.

robousy
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Hi,

I am interested in what I can DO with the stress energy tensor once I've obtained it from a metric.

I am not so interested in the formal development, just a book or paper that shows what its good for.

I am interested in cosmology, specifically: brane worlds, brane gas cosmology, stability of compact extra dimensions and the casimir effect.

If anyone can recommend a good pedagogical source not too dense in formalism then I'd like very much to hear from you!

:smile:
 
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Essentially what you have obtained is the "distribution of the matter content" [in terms of "matter fields"] obtained from the geometry. Probably the first thing you should do is to check that the stress energy is physically reasonable. Check whether it satisfies the "energy conditions" (See, e.g., http://en.wikipedia.org/wiki/Energy_conditions ).
 
By appropriately contracting the stress-energy tensor with the 4-velocity (field) of some observer, you'll find the local energy and momentum densities of the matter that are seen by that person. You'll also get the stress tensor he observes (as it is usually defined in Newtonian treatments of elasticity and fluid mechanics). Any GR text should explain this.
 

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