A semi-classical relativistic black hole
| dc.creator | Vendrell, F. | |
| dc.date | 1996-08-01 | |
| dc.date.accessioned | 2026-07-07T04:22:19Z | |
| dc.date.available | 2026-07-07T04:22:19Z | |
| dc.description | A new two-dimensional black hole model, based on the "R=T" relativistic theory, is introduced, and the quantum massless scalar field is studied in its classical gravitational field. In particular infrared questions are discussed. The two-point function, energy-momentum tensor, current, Bogoliubov transformations and the mean number of created particles for a given test function are computed. I show that this black hole emits massless scalar particles spontaneously. Comparison with the corresponding field theory in a thermal bath shows that the spontaneous emission is everywhere thermal, i.e. not only near the horizon. | |
| dc.description | 34 pages | |
| dc.identifier | https://arxiv.org/abs/hep-th/9608007 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9608007 | |
| dc.identifier | Helv.Phys.Acta 70 (1997) 598-635 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54673 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | A semi-classical relativistic black hole | |
| dc.type | text |