A black hole in two-dimensional space-time
| dc.creator | Vendrell, F. | |
| dc.date | 1997-05-19 | |
| dc.date.accessioned | 2026-07-07T04:23:20Z | |
| dc.date.available | 2026-07-07T04:23:20Z | |
| dc.description | An imploding shell of radiation is shown to create a 2-D black hole within the framework of the ``R=T'' theory. The radius of the horizon is given by 1/(2M), where M is the mass of the black hole. The topology of the central singularity is that of a corner. The radiation emitted very far from the black hole is thermal with temperature M/(2π). The back-reaction problem is solved to one-loop order. | |
| dc.description | 12 pages, Revtex, 2 figures | |
| dc.identifier | https://arxiv.org/abs/hep-th/9705135 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9705135 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54989 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A black hole in two-dimensional space-time | |
| dc.type | text |