Phase transition for black holes with scalar hair and topological black holes

被引:37
作者
Myung, Yun Soo [1 ,2 ]
机构
[1] Inje Univ, Inst Basic Sci, Gimhae 621749, South Korea
[2] Inje Univ, Sch Comp Aided Sci, Gimhae 621749, South Korea
关键词
D O I
10.1016/j.physletb.2008.03.046
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study phase transitions between black holes with scalar hair and topological black holes in asymptotically anti-de Sitter spacetimes. As the ground state solutions, we introduce the non-rotating BTZ black hole in three dimensions and topological black hole with hyperbolic horizon in four dimensions. For the temperature matching only, we show that the phase transition between black hole with scalar hair (Martinez-Troncoso-Zanelli black hole) and topological black hole is second-order by using differences between two free energies. However, we do not identify what order of the phase transition between scalar and non-rotating BTZ black holes occurs in three dimensions, although there exists a possible decay of scalar black hole to non-rotating BTZ black hole. (C) 2008 Elsevier B.V. All rights reserved.
引用
收藏
页码:111 / 117
页数:7
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