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arXiv · 0801.3163

Anti-de Sitter Quotients: When Are They Black Holes?

Stefan Aminneborg·Ingemar Bengtsson
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Abstract

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 scri 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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Stefan Aminneborg, Ingemar Bengtsson. 2008-04-23. Anti-de Sitter Quotients: When Are They Black Holes?. https://doi.org/10.1088/0264-9381%2F25%2F9%2F095019

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