Anti-de Sitter Quotients: When Are They Black Holes?
| dc.creator | Aminneborg, Stefan | |
| dc.creator | Bengtsson, Ingemar | |
| dc.date | 2008-01-21 | |
| dc.date | 2008-04-23 | |
| dc.date.accessioned | 2026-07-07T11:14:06Z | |
| dc.date.available | 2026-07-07T11:14:06Z | |
| dc.description | 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. | |
| dc.description | 16 pages, 4 figures; minor polish added | |
| dc.identifier | https://arxiv.org/abs/0801.3163 | |
| dc.identifier | http://arxiv.org/abs/0801.3163 | |
| dc.identifier | Class.Quant.Grav.25:095019,2008 | |
| dc.identifier | doi:10.1088/0264-9381/25/9/095019 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/191951 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Anti-de Sitter Quotients: When Are They Black Holes? | |
| dc.type | text |