The nature of singularity in Bianchi I cosmological string gravity model with second order curvature corrections

被引:19
作者
Alexeyev, S [1 ]
Toporensky, A [1 ]
Ustiansky, V [1 ]
机构
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1016/S0370-2693(01)00556-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate Bianchi I cosmological model in the theory of a dilaton field coupled to gravity through a Gauss-Bonnet term. Two type of cosmological singularity are distinguished. The former is analogous to the Einstein gravity singularity, the latter (which does not appear in classical General Relativity) occurs when the main determinant of the system of field equations vanishes. An analogy between the latter cosmological singularity and the singularity inside a black hole with a dilatonic hair is discussed. Initial conditions, leading to these two types of cosmological singularity are found via numerical integration of the equation of motion. (C) 2001 Published by Elsevier Science B.V.
引用
收藏
页码:151 / 156
页数:6
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