Phase transitions near black hole horizons

被引:146
作者
Gubser, SS [1 ]
机构
[1] Princeton Univ, Joseph Henry Labs, Princeton, NJ 08544 USA
关键词
D O I
10.1088/0264-9381/22/23/013
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Reissner-Nordstrom black hole in four dimensions can be made unstable without violating the dominant energy condition by introducing a real massive scalar with non-renormalizable interactions with the gauge field. New stable black hole solutions then exist with greater entropy for fixed mass and charge than the Reissner-Nordstrom solution. In these new solutions, the scalar condenses to a non-zero value near the horizon. Various generalizations of these hairy black holes are discussed, and an attempt is made to characterize when black hole hair can occur.
引用
收藏
页码:5121 / 5143
页数:23
相关论文
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