Adiabatic models of the cosmological radiative era

DOI10.1023/A:1020164005579zbMath1025.83033arXivgr-qc/0111010OpenAlexW1558171772WikidataQ125375074 ScholiaQ125375074MaRDI QIDQ1863093

Mustapha Ishak, Roberto A. Sussman

Publication date: 11 March 2003

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0111010

zbMATH Keywords

adiabatic perturbationsEarly Universeexact solution to Einstein's equationsisotropic Friedmann universeLemaître-Tolman-Bondi solution

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

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• Anisotropic solutions of the Einstein-Boltzmann equations. I: General formalism
• Anisotropic solutions of the Einstein-Boltzmann equations. II: Some exact properties of the equations
• Relaxation versus collision times in the cosmological radiative era
• Ideal gas sources for the Lemaître-Tolman-Bondi metrics
• Cosmological Physics
• Exact solutions of Einstein's equations with ideal gas sources
• Inhomogeneous Cosmological Models
• Does the isotropy of the CMB imply a homogeneous universe? Some generalized EGS theorems

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