Quantum Dust Black Holes
| dc.creator | Peleg, Yoav | |
| dc.date | 1993-07-08 | |
| dc.date.accessioned | 2026-07-07T04:19:32Z | |
| dc.date.available | 2026-07-07T04:19:32Z | |
| dc.description | By analysing the infinite dimensional midisuperspace of spherically symmetric dust universes, and aply it to collapsing dust stars, one finds that the general quantum state is a bound state. This leads to discrete spectrum. In the case of a Schwarzschild black hole, the discrete spectrum implies Bekenstein area quantization: the area of the horizon is an integer multiple of the Planck area. Knowing the microscopic (quantum) states, we suggest a microscopic interpretation of the thermodynamics of black holes: the degeneracy of the quantum states forming a black hole, gives the Bekenstein- Hawking entropy. All other thermodynamical quantities can be derived by using the standard definitions. | |
| dc.description | 30 pages, BRX-TH-350 | |
| dc.identifier | https://arxiv.org/abs/hep-th/9307057 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9307057 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/53589 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Quantum Dust Black Holes | |
| dc.type | text |