Decompactification near the horizon and non-vanishing entropy
| dc.creator | Behrndt, Klaus | |
| dc.date | 1996-11-28 | |
| dc.date.accessioned | 2026-07-07T04:22:53Z | |
| dc.date.available | 2026-07-07T04:22:53Z | |
| dc.description | Intersecting D-brane configurations are related to black holes in D=4. Using the standard way of compactification only the Reissner-Nordstrøm black hole is non-singular. In this paper we argue, that also the other black holes are non-singular if i) we compactify over a periodic array and ii) we allow the string metric after reaching a critical curvature to choose the dual geometry. Effectively this means that near the horizon the solution completely decompactifies and chooses a non-singular D-brane configuration. | |
| dc.description | (hyper) Latex, 7 pages, Contribution for STRINGS96(black holes) | |
| dc.identifier | https://arxiv.org/abs/hep-th/9611237 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9611237 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54824 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Decompactification near the horizon and non-vanishing entropy | |
| dc.type | text |