Black hole entropy quantization
| dc.creator | Corichi, Alejandro | |
| dc.creator | Diaz-Polo, Jacobo | |
| dc.creator | Fernandez-Borja, Enrique | |
| dc.date | 2006-09-26 | |
| dc.date | 2007-05-01 | |
| dc.date.accessioned | 2026-07-07T11:04:31Z | |
| dc.date.available | 2026-07-07T11:04:31Z | |
| dc.description | Ever since the pioneer works of Bekenstein and Hawking, black hole entropy has been known to have a quantum origin. Furthermore, it has long been argued by Bekenstein that entropy should be quantized in discrete (equidistant) steps given its identification with horizon area in (semi-)classical general relativity and the properties of area as an adiabatic invariant. This lead to the suggestion that black hole area should also be quantized in equidistant steps to account for the discrete black hole entropy. Here we shall show that loop quantum gravity, in which area is {\it not} quantized in equidistant steps can nevertheless be consistent with Bekenstein's equidistant entropy proposal in a subtle way. For that we perform a detailed analysis of the number of microstates compatible with a given area and show consistency with the Bekenstein framework when an oscillatory behavior in the entropy-area relation is properly interpreted. | |
| dc.description | 4 pages, 4 figures. Version to be published in PRL | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0609122 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0609122 | |
| dc.identifier | Phys.Rev.Lett.98:181301,2007 | |
| dc.identifier | doi:10.1103/PhysRevLett.98.181301 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/188919 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Black hole entropy quantization | |
| dc.type | text |