Comment about quasiisotropic solution of Einstein equations near cosmological singularity

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  • 12 April 2002
Abstract
We generalize for the case of arbitrary hydrodynamical matter the quasiisotropic 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 quasiisotropic expansion acquires a more complicated form.

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