Radiation Ball as a Black Hole
| dc.creator | Nagatani, Yukinori | |
| dc.date | 2003-10-20 | |
| dc.date | 2003-12-07 | |
| dc.date.accessioned | 2026-07-07T04:16:02Z | |
| dc.date.available | 2026-07-07T04:16:02Z | |
| dc.description | A structure of the radiation-ball which is identified as a Schwarzschild black hole is found out by investigating the backreaction of Hawking radiation into space-time. The structure consists of the radiation which is gravitationally bounded in the ball and of a singularity. The entropy of the radiation in the ball is proportional to the surface-area of the ball and nearly equals to the Bekenstein entropy. The Hawking radiation is regarded as a leak-out from the ball. There arises no information paradox because there exists no horizon in the structure. | |
| dc.description | 12 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/hep-th/0310185 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0310185 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/52189 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Radiation Ball as a Black Hole | |
| dc.type | text |