Quantum spectrum of black holes
| dc.creator | Kiselev, V. V. | |
| dc.date | 2005-09-12 | |
| dc.date | 2005-10-03 | |
| dc.date.accessioned | 2026-07-07T06:20:23Z | |
| dc.date.available | 2026-07-07T06:20:23Z | |
| dc.description | The black hole as the thermodynamical system in equilibrium possesses the periodicity of motion in imaginary time, that allows us to formulate the quasi-classical rule of quantization. The rule yields the equidistant spectrum for the entropy of non-rotating black holes as well as for the appropriately scaled entropy in the case of rotation. We clarify and discuss a role of quasi-normal modes. | |
| dc.description | 5 pages, RevTeX4 class; v2, v3: references added | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0509038 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0509038 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/95315 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Quantum spectrum of black holes | |
| dc.type | text |