Comment about quasi-isotropic solution of Einstein equations near cosmological singularity

Preprint

20 April 2002

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/0204045

Abstract

We generalize for the case of arbitrary hydrodynamical matter the quasi-isotropic solution of Einstein equations near cosmological singularity, found by Lifshitz and Khalatnikov in 1960 for the case of radiation-dominated universe. It is shown that this solution always exists, but dependence of terms in the quasi-isotropic expansion acquires a more complicated form.

Keywords

QUASI ISOTROPIC SOLUTION
COSMOLOGICAL SINGULARITY
SOLUTION OF EINSTEIN
EINSTEIN EQUATIONS
SINGULARITY

All Related Versions

Version 1, 2002-04-12, ArXiv
Version 2, 2002-04-20, ArXiv
Published version: Classical and Quantum Gravity, 19 (14), 3845.

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