Note on self-gravitating radiation in AdS spacetime
文献类型：期刊论文
| 作者 | Hu, Bin; Li, Zhong-Hua; Cai, Rong-Gen ; Li, ZH , China W Normal Univ, Dept Phys, Nanchong 637002, Peoples R China
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| 刊名 | PHYSICAL REVIEW D
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| 出版日期 | 2008 |
| 卷号 | 77期号:10页码:- |
| ISSN号 | 1550-7998 |
| 关键词 | 3-dimensional Black-holes De-sitter Space General-relativity Thermodynamics |
| 英文摘要 | Recently Vaganov and Hammersley investigated independently the equilibrium self-gravitating radiation in higher (d >= 4)-dimensional, spherically symmetric anti-de Sitter space. It was found that in 4 <= d <= 10, there exist locally stable radiation configurations all the way up to a maximum red-shifted temperature, above which there are no solutions; there is also a maximum mass and maximum entropy configuration occurring at a higher central density than the maximal temperature configuration. Beyond their peaks the temperature, mass, and entropy undergo an infinite series of damped oscillations, which indicates the configurations in this range are unstable. In d >= 11, the temperature, mass, and entropy of the self-gravitating configuration are monotonic functions of the central energy density, asymptoting to their maxima as the central density goes to infinity. In this paper we investigate the equilibrium self-gravitating radiation in higher-dimensional, plane-symmetric anti-de Sitter space. We find that there exist essential differences from the spherically syrnmetric case: In each dimension (d >= 4), there are maximal mass (density), maximal entropy (density), and maximal temperature configurations; they do not appear at the same central energy density; the oscillation behavior appearing in the spherically symmetric case does not happen in this case; and the mass (density), as a function of the central energy density, increases first and reaches its maximum at a certain central energy density and then decreases monotonically in 4 <= d <= 7, while in d >= 8, besides the maximum, the mass (density) of the equilibrium configuration has a minimum: the mass (density) first increases and reaches its maximum, then decreases to its minimum, and then increases to its asymptotic value monotonically. The reason causing the difference is discussed. |
| 学科主题 | Physics |
| URL标识 | 查看原文 |
| WOS记录号 | WOS:000257329300076 |
| 公开日期 | 2012-08-02 |
| 源URL | [http://ir.itp.ac.cn/handle/311006/5538]  |
| 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 | Li, ZH , China W Normal Univ, Dept Phys, Nanchong 637002, Peoples R China |
| 推荐引用方式 GB/T 7714 | Hu, Bin,Li, Zhong-Hua,Cai, Rong-Gen,et al. Note on self-gravitating radiation in AdS spacetime[J]. PHYSICAL REVIEW D,2008,77(10):-. |
| APA | Hu, Bin,Li, Zhong-Hua,Cai, Rong-Gen,&Li, ZH , China W Normal Univ, Dept Phys, Nanchong 637002, Peoples R China.(2008).Note on self-gravitating radiation in AdS spacetime.PHYSICAL REVIEW D,77(10),-. |
| MLA | Hu, Bin,et al."Note on self-gravitating radiation in AdS spacetime".PHYSICAL REVIEW D 77.10(2008):-. |
入库方式： OAI收割
来源：理论物理研究所
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