Theories without the use of cosmological principle.

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SUMMARY

The discussion centers on the existence of cosmological theories that do not utilize the cosmological principle. It highlights inhomogeneous and anisotropic models such as the Lemaitre-Tolman-Bondi dust and the Oppenheimer-Snyder collapsing ball. Despite these models, the empirical evidence supporting the cosmological principle remains robust, with observations like the large-scale distribution of matter, Cosmic Microwave Background (CMB), and peculiar velocities serving as significant proofs. The conversation concludes that while alternative models exist, they are often viewed as equivalent to the standard cosmological model at observable scales.

PREREQUISITES
  • Understanding of the cosmological principle
  • Familiarity with inhomogeneous and anisotropic cosmological models
  • Knowledge of observational cosmology, including CMB and galaxy distribution
  • Basic grasp of inflationary theory in cosmology
NEXT STEPS
  • Research the Lemaitre-Tolman-Bondi dust model in detail
  • Explore the implications of the Oppenheimer-Snyder collapsing ball model
  • Investigate the role of the Cosmic Microwave Background (CMB) in supporting the cosmological principle
  • Study the effects of inhomogeneity and anisotropy in the context of inflationary cosmology
USEFUL FOR

Astronomers, cosmologists, and physics students interested in alternative cosmological models and the implications of the cosmological principle on large-scale structures in the universe.

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are there theories in cosmology which do not incorporate/use the cosmological principle?
 
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There are some inhomogeneous and anisotropic cosmological models that were analyzed and studied in past, like the Lemaitre-Tolman-Bondi dust, the Oppenheimer-Snyder collapsing ball, etc. But in the meanwhile the empirical support of the cosmological principle is strong and there are lots of phenomena that are considered proofs of it, e.g. large scale distribution of matter (galaxies, quasars), CMB, X-ray background, peculiar velocities, etc. IMO the only way to take some of these models seriously is to assume that they are equivalent to the standard cosmological model at observable scales, for example like this one. This would shift a little bit your question to whether there are currently cosmological models in which there is assumed inhomogeneity or anisotropy at very large scales. The answer to this is yes, even within the standard cosmological model the cosmological principle is not expected to apply at arbitrary large scales because of the finite size of our inflationary bubble.
 

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