Self-gravitating fluid systems and galactic dark matter

被引:7
|
作者
Banik, Uddipan [1 ]
Dey, Dipanjan [1 ]
Bhattacharya, Kaushik [1 ]
Sarkar, Tapobrata [1 ]
机构
[1] Indian Inst Technol, Dept Phys, Kanpur 208016, Uttar Pradesh, India
关键词
Gravitational collapse; Dark matter; Relativistic fluids; Newtonian fluids; GALAXIES; COLLAPSE;
D O I
10.1007/s10714-017-2284-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study gravitational collapsewith anisotropic pressures, whose end stage can mimic space-times that are seeded by galactic dark matter. To this end, we identify a class of space-times (with conical defects) that can arise out of such a collapse process, and admit stable circular orbits at all radial distances. These have a naked singularity at the origin. An example of such a space-time is seen to be the Bertrand space-time discovered by Perlick, that admits closed, stable orbits at all radii. Using relativistic two-fluid models, we show that our galactic space-times might indicate exotic matter, i.e one of the component fluids may have negative pressure for a certain asymptotic fall off of the associated mass density, in the Newtonian limit. We complement this analysis by studying some simple examples of Newtonian two-fluid systems, and compare this with the Newtonian limit of the relativistic systems considered.
引用
收藏
页数:21
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