Radiating star, shear-free gravitational collapse without horizon

被引：19

作者：

Tewari, B. C. ^{[1
]}

Charan, Kali ^{[1
]}

机构：

[1] Kumaun Univ, Dept Math, Almora, India

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2014年 / 351卷 / 02期

关键词：

Exact solutions; Radiating star; Gravitational collapse; Naked singularity; SPHERES;

D O I：

10.1007/s10509-014-1851-9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a new model of dissipative energy fluid without appearance of horizon. The interior matter fluid is shear-free isotropic spherically symmetric and undergoing radial heat flow. The interior metric is matched with Vaidya exterior metric over the boundary. The model obeyed all the relevant physical and thermodynamic conditions. In this model, the collapse begins at infinite past with both infinite mass and radius and contracts to a point as time tends to zero without forming an event horizon.

引用

页码：613 / 617

页数：5

共 45 条

[1]

[Anonymous], 1951, P INDIAN ACAD SCI A

[2] CONFORMALLY FLAT SOLUTION WITH HEAT-FLUX [J].