On horizon constraints and Hawking radiation
| dc.creator | Mattingly, David | |
| dc.date | 2006-01-11 | |
| dc.date.accessioned | 2026-07-07T06:58:03Z | |
| dc.date.available | 2026-07-07T06:58:03Z | |
| dc.description | Questions about black holes in quantum gravity generally presuppose the presence of a horizon. Recently Carlip has shown that enforcing an initial data surface to be a horizon leads to the correct form for the Bekenstein-Hawking entropy of the black hole. Requiring a horizon also constitutes fixed background geometry, which generically leads to non-conservation of the matter stress tensor at the horizon. In this work, I show that the generated matter energy flux for a Schwarzschild black hole is in agreement with the first law of black hole thermodynamics, $8 πG ΔQ = κΔA$. | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0601044 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0601044 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/107206 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | On horizon constraints and Hawking radiation | |
| dc.type | text |