Anti-de Sitter quotients:: when are they black holes?

被引：4
作者：
Aminneborg, Stefan [1 ]
Bengtsson, Ingemar [2 ]
机构：
[1] Norra Reals Gymnasium, S-11355 Stockholm, Sweden
[2] Stockholm Univ, S-10691 Stockholm, Sweden
来源：
CLASSICAL AND QUANTUM GRAVITY | 2008年 / 25卷 / 09期
关键词：
D O I：
10.1088/0264-9381/25/9/095019
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We point out that the BTZ black holes, and their relatives, can be defined in a cleaner way than they originally were. The covering space can be taken to be anti-de Sitter space, period, while I splits up into components due to Misner singularities. Our definition permits us to choose between two conflicting claims concerning BTZ black holes in (3 + 1) dimensions.
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收藏
页数：10
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