What is the fate of a black hole embedded in an expanding universe?

被引：33
|
作者：
Faraoni, Valerio [1 ]
Gao, Changjun [2 ]
Chen, Xuelei [2 ]
Shen, You-Gen [3 ,4 ,5 ]
机构：
[1] Bishops Univ, Dept Phys, 2600 Coll Sr, Sherbrooke, PQ J1M 1Z7, Canada
[2] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[3] Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
[4] Joint Inst Galaxy & Cosmol SHAO, Shanghai 200030, Peoples R China
[5] USTC, Shanghai 200030, Peoples R China
来源：
PHYSICS LETTERS B | 2009年 / 671卷 / 01期
基金：
加拿大自然科学与工程研究理事会; 美国国家科学基金会;
关键词：
Black holes in cosmological backgrounds; Time-dependent horizons; ISOLATED HORIZONS; GRAVITATIONAL-RADIATION; ISOTROPIC UNIVERSE; POINT MASS; ENERGY; LAWS; AREA;
D O I：
10.1016/j.physletb.2008.11.067
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Within a large class of exact solutions of the Einstein equations describing a black hole embedded in a Friedmann universe it is shown that, under certain assumptions, Only those with comoving Hawking-Hayward quasi-local mass are generic, in the sense that they are late-time attractors. (C) 2008 Elsevier B.V. All rights reserved.
引用
收藏
页码：7 / 9
页数：3
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