Notes on a quantum gravitational collaps
| dc.creator | Berezin, Victor | |
| dc.date | 2000-12-30 | |
| dc.date.accessioned | 2026-07-07T03:25:34Z | |
| dc.date.available | 2026-07-07T03:25:34Z | |
| dc.description | Everybody knows what the classical black holes are. In short, this is a spacetime region beyond the so-called event horizon. The notion of the event horizon is mathematically well defined. The situation with a definition of quantum black hole is not so clear. The problem is that the classical event horizon can be defined only globally, i.e. in order to be sure we have a black hole we would need an infinite time interval. But, in classical physics we have trajectories off all the particles and equations of motion for all the fields and can, in principle, construct some ideal models for the gravitational collapse and study the black hole formation under different conditions. | |
| dc.description | The Ninth Marcel Grossmann Meeting | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0101004 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0101004 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33760 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Notes on a quantum gravitational collaps | |
| dc.type | text |