Physical nature of the central singularity in spherical collapse

被引:53
作者
Deshingkar, SS [1 ]
Joshi, PS [1 ]
Dwivedi, IH [1 ]
机构
[1] Tata Inst Fundamental Res, Theoret Astrophys Grp, Bombay 400005, Maharashtra, India
来源
PHYSICAL REVIEW D | 1999年 / 59卷 / 04期
关键词
D O I
10.1103/PhysRevD.59.044018
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine here the nature of the central singularity forming in the spherically symmetric collapse of a dust cloud and it is shown that this is always a strong curvature singularity where gravitational tidal forces diverge powerfully. An important consequence is that the nature of the naked singularity forming in the dust collapse turns out to be stable against the perturbations in the initial data from which the collapse commences. [S0556-2821(99)02002-0].
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页数:6
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