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Anti-de Sitter Quotients: When Are They Black Holes?
Stockholm University, Faculty of Science, Department of Physics. (KoF)
2008 (English)In: Classical and quantum gravity, ISSN 0264-9381, E-ISSN 1361-6382, Vol. 25, 095019- p.Article in journal (Refereed) Published
Abstract [en]

e 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 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.

Place, publisher, year, edition, pages
2008. Vol. 25, 095019- p.
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Other Physics Topics
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Physics
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URN: urn:nbn:se:su:diva-33791ISI: 000255897000020OAI: oai:DiVA.org:su-33791DiVA: diva2:283592
Available from: 2009-12-29 Created: 2009-12-29 Last updated: 2011-07-06Bibliographically approved

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