Black hole formation from collapsing dust fluid in a background of dark energy
文献类型:期刊论文
作者 | Wang, AZ; Cai, RG![]() |
刊名 | PHYSICAL REVIEW D
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出版日期 | 2006 |
卷号 | 73期号:6页码:- |
关键词 | Digital Sky Survey Probe Wmap Observations Galaxy Redshift Survey General Relativity Gravitational Collapse Cosmological Constant Scalar Field Data Release White Holes Universe |
ISSN号 | 1550-7998 |
英文摘要 | The gravitational collapse of a spherically symmetric star, made of a dust fluid, rho(DM), in a background of dark energy, p=w rho (w <-1/3) is studied. It is found that when only dark energy is present, black holes are never formed. When both of them are present, black holes can be formed, due to the condensation of the dust fluid. Initially the dust fluid may not play an important role, but, as time increases, it will dominate the collapse and finally lead to formation of black holes. This result remains true even when the interaction between the dust fluid and dark energy does not vanish. When w <-1 (phantoms), some models also can be interpreted as representing the death of a white hole that ejects both dust and phantoms. The ejected matter recollapses to form a black hole. |
学科主题 | Physics |
URL标识 | 查看原文 |
WOS记录号 | WOS:000236466100010 |
公开日期 | 2012-08-02 |
源URL | [http://ir.itp.ac.cn/handle/311006/6027] ![]() |
专题 | 理论物理研究所_理论物理所1978-2010年知识产出 |
通讯作者 | Cai, RG , Chinese Acad Sci, Inst Theoret Phys, POB 2735, Beijing 100080, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, AZ,Cai, RG,Cai, RG , Chinese Acad Sci, Inst Theoret Phys, POB 2735, Beijing 100080, Peoples R China. Black hole formation from collapsing dust fluid in a background of dark energy[J]. PHYSICAL REVIEW D,2006,73(6):-. |
APA | Wang, AZ,Cai, RG,&Cai, RG , Chinese Acad Sci, Inst Theoret Phys, POB 2735, Beijing 100080, Peoples R China.(2006).Black hole formation from collapsing dust fluid in a background of dark energy.PHYSICAL REVIEW D,73(6),-. |
MLA | Wang, AZ,et al."Black hole formation from collapsing dust fluid in a background of dark energy".PHYSICAL REVIEW D 73.6(2006):-. |
入库方式: OAI收割
来源:理论物理研究所
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