What role do pressures play in determining the final end state of gravitational collapse?

被引:41
作者
Goswami, R [1 ]
Joshi, PS [1 ]
机构
[1] Tata Inst Fundamental Res, Dept Astron & Astrophys, Bombay 400005, Maharashtra, India
关键词
D O I
10.1088/0264-9381/19/20/314
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine here in what way pressures affect the final fate of a continual gravitational collapse. It is shown that the presence of a non-vanishing pressure gradient in the collapsing cloud can determine directly the epoch of formation of trapped surfaces and the apparent horizon, thus changing the causal structure in the vicinity of a singularity.
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收藏
页码:5229 / 5234
页数:6
相关论文
共 9 条
  • [1] CELERIER M, 2002, GRQC0203094
  • [2] GIAMBO R, 2002, GRQC0204030
  • [3] Physical processes in naked singularity formation
    Harada, T
    Iguchi, H
    Nakano, KI
    [J]. PROGRESS OF THEORETICAL PHYSICS, 2002, 107 (03): : 449 - 524
  • [4] Hawking S. W., 1973, The Large Scale Structure of Space-Time
  • [5] Local anisotropy in self-gravitating systems
    Herrera, L
    Santos, NO
    [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1997, 286 (02): : 53 - 130
  • [6] Joshi P. S., 1993, GLOBAL ASPECTS GRAVI
  • [7] Initial data and the end state of spherically symmetric gravitational collapse
    Joshi, PS
    Dwivedi, IH
    [J]. CLASSICAL AND QUANTUM GRAVITY, 1999, 16 (01) : 41 - 59
  • [8] Why do naked singularities form in gravitational collapse?
    Joshi, PS
    Dadhich, N
    Maartens, R
    [J]. PHYSICAL REVIEW D, 2002, 65 (10)
  • [9] ZUMHAGEN HM, 1974, COMMUN MATH PHYS, V37, P29