Generalized second law and entropy bound for a Reissner- Nordström black hole
| dc.creator | Kuriakose, P. I. | |
| dc.creator | Kuriakose, V. C. | |
| dc.date | 2008-06-13 | |
| dc.date.accessioned | 2026-07-07T09:44:28Z | |
| dc.date.available | 2026-07-07T09:44:28Z | |
| dc.description | It has been conjectured that black hole interacting with its surroundings will obey the Generalized Second Law ($GSL$) of thermodynamics. Conservation of $GSL$ is due to the fully thermal nature of Hawking radiation and an upper bound on entropy. We study these aspects for a Reissner-Nordstr$\ddot{\textbf{o}}$m ($RN$)black hole and conjecture that $GSL$ may be conserved if the equation of state of radiation near the horizon is modified. An upper bound on $S/E$, similar to the Bekenstein form evolves in the calculation. | |
| dc.description | 11 pages | |
| dc.identifier | https://arxiv.org/abs/0806.2192 | |
| dc.identifier | http://arxiv.org/abs/0806.2192 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/162887 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Generalized second law and entropy bound for a Reissner- Nordström black hole | |
| dc.type | text |