抄録
We analyze the effects of the back reaction due to a conformal field theory (CFT) on a black hole spacetime with negative cosmological constant. We study the geometry numerically and take into account the energy momentum tensor of CFT approximated by a radiation fluid. We find a sequence of configurations without a horizon in thermal equilibrium (CFT stars), followed by a sequence of configurations with a horizon. We discuss the thermodynamic properties of the system and how back reaction effects alter the space-time structure. We also provide an interpretation of the above sequence of solutions in terms of the AdS/CFT correspondence. The dual five-dimensional description is given by the Karch-Randall model, in which a sequence of five-dimensional floating black holes followed by a sequence of brane localized black holes correspond to the above solutions.
本文言語 | 英語 |
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ページ | 177-180 |
ページ数 | 4 |
出版ステータス | 出版済み - 12月 1 2009 |
外部発表 | はい |
イベント | 19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009 - Tokyo, 日本 継続期間: 11月 30 2009 → 12月 4 2009 |
その他
その他 | 19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009 |
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国/地域 | 日本 |
City | Tokyo |
Period | 11/30/09 → 12/4/09 |
!!!All Science Journal Classification (ASJC) codes
- 原子分子物理学および光学