Black hole entropy from a single long string
| dc.creator | Oda, Ichiro | |
| dc.date | 1996-06-07 | |
| dc.date.accessioned | 2026-07-07T04:22:08Z | |
| dc.date.available | 2026-07-07T04:22:08Z | |
| dc.description | In this article we derive the Bekenstein-Hawking formula of black hole entropy from a single string. We consider a open string in the Rindler metric which can be obtained in the large mass limit from the Schwarzschild black hole metric. By solving the field equations we find a nontrivial solution with the exact value of the Hawking temperature. We see that this solution gives us the Bekenstein-Hawking formula of black hole entropy to leading order of approximation. This string has effectively a rescaled string tension having a relation with a redshift factor. It is also pointed out that this formalism is extensible to other black holes in an arbitrary spacetime dimension. The present work might lead us to a surprising idea that the recent picture which the black hole entropy arises from D-brane excitations has the root of the picture that the black hole entropy is stocked in a single long string with a rescaled string tension. | |
| dc.description | 9 pages, phyzzx | |
| dc.identifier | https://arxiv.org/abs/hep-th/9606035 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9606035 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54599 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Black hole entropy from a single long string | |
| dc.type | text |