Classical black hole evaporation in Randall-Sundrum infinite braneworld
| dc.creator | Tanaka, Takahiro | |
| dc.date | 2002-03-24 | |
| dc.date | 2002-04-03 | |
| dc.date.accessioned | 2026-07-07T11:08:38Z | |
| dc.date.available | 2026-07-07T11:08:38Z | |
| dc.description | After the gravity induced on the brane in the Randall-Sundrum (RS) infinite braneworld is briefly reviewed, we discuss the possibility that black holes evaporate as a result of classical evolution in this model based on the AdS/CFT correspondence. If this possibility is really the case, the existence of long-lived solar mass black holes will give the strongest constraint on the bulk curvature radius. At the same time, we can propose a new method to simulate the evaporation of a 4D black hole due to the Hawking radiation as a 5D process. | |
| dc.description | Style file changed, Proceedings for YITP workshop "Braneworld -Dynamics of spacetime boundary" | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0203082 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0203082 | |
| dc.identifier | Prog.Theor.Phys.Suppl.148:307-316,2003 | |
| dc.identifier | doi:10.1143/PTPS.148.307 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/190202 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Classical black hole evaporation in Randall-Sundrum infinite braneworld | |
| dc.type | text |