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

被引：36

作者：

Khalatnikov, IM

Kamenshchik, AY

Starobinsky, AA

机构：

[1] Russian Acad Sci, LD Landau Inst Theoret Phys, Moscow 117334, Russia

[2] Landau Network Ctr Volta, I-22100 Como, Italy

[3] Tel Aviv Univ, Sch Phys & Astron, Raymond & Sackler Fac Exact Sci, IL-69978 Tel Aviv, Israel

来源：

CLASSICAL AND QUANTUM GRAVITY | 2002年 / 19卷 / 14期

关键词：

D O I：

10.1088/0264-9381/19/14/322

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

For the case of arbitrary hydrodynamical matter, we generalize the quasi-isotropic solution of Einstein equations near the cosmological singularity, found by Lifshitz and Khalatnikov in 1960 for the case of the 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.

引用

页码：3845 / 3849

页数：5

共 17 条

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