RADIATING GRAVITATIONAL COLLAPSE WITH BULK VISCOSITY

被引：16

作者：

MARTINEZ, J

PAVON, D

机构：

[1] Departamento de Física, Grupo de Física Estadística, Universidad Autónoma de Barcelona, Bellaterra, Barcelona

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1994年 / 268卷 / 03期

关键词：

GRAVITATION; RADIATIVE TRANSFER; RELATIVITY; STARS; MASS-LOSS; NEUTRON; WHITE DWARFS;

D O I：

10.1093/mnras/268.3.654

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The complete gravitational collapse of a spherically symmetric dense star with an outgoing radial heat flow and a dissipative bulk pressure is studied. The behaviour of the luminosity, temperature, sound speed and adiabatic index is analysed. The neutrino trapping in the core of the star in the last phases of the collapse makes the bulk pressure non-negligible as measured against the hydrostatic pressure. Our work generalizes that of some previous authors.

引用

页码：654 / 664

页数：11

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