Gravitational demise of cold degenerate stars

被引：9

作者：

Adams, FC ^{[1
]}

Laughlin, G

Mbonye, M

Perry, MJ

机构：

[1] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[2] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 9EW, England

来源：

PHYSICAL REVIEW D | 1998年 / 58卷 / 08期

关键词：

D O I：

10.1103/PhysRevD.58.083003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We consider the long term fate and evolution of cold degenerate stars under the action of gravity alone. Although such stars cannot emit radiation through the Hawking mechanism, the wave function of the star will contain a small admixture of black hole states. These black hole states will emit radiation and hence the star can lose its mass energy in the long term. We discuss the allowed range of possible degenerate stellar evolution within this framework. [S0556-2821(98)00222-7].

引用

页数：7

共 21 条

[1] A dying universe: The long-term fate and evolution of astrophysical objects [J].