Possible black universes in a brane world

被引:3
|
作者
Bronnikov, K. A. [1 ,2 ]
Donskoy, E. V. [2 ]
机构
[1] VNIIMS, Ctr Gravitat & Fundamental Metrol, Moscow 117361, Russia
[2] PFUR, Inst Gravitat & Cosmol, Moscow 117198, Russia
来源
GRAVITATION & COSMOLOGY | 2010年 / 16卷 / 01期
基金
俄罗斯基础研究基金会;
关键词
DARK ENERGY; HOLES;
D O I
10.1134/S0202289310010068
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A black universe is a nonsingular black hole where, beyond the horizon, there is an expanding, asymptotically isotropic universe. Such spherically symmetric configurations have been recently found as solutions to the Einstein equations with phantom scalar fields (with negative kinetic energy) as sources of gravity. They have a Schwarzschild-like causal structure but a de Sitter infinity instead of a singularity. It is attempted to obtain similar configurations without phantoms, in the framework of an RS2 type brane world scenario, considering the modified Einstein equations that describe gravity on the brane. By building an explicit example, it is shown that black-universe solutions can be obtained there in the presence of a scalar field with positive kinetic energy and a nonzero potential.
引用
收藏
页码:42 / 49
页数:8
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