Hawking Radiation from General Kerr-(anti)de Sitter Black Holes
| dc.creator | Xu, Zhibo | |
| dc.creator | Chen, Bin | |
| dc.date | 2006-12-25 | |
| dc.date | 2007-01-27 | |
| dc.date.accessioned | 2026-07-07T11:23:30Z | |
| dc.date.available | 2026-07-07T11:23:30Z | |
| dc.description | We calculate the total flux of Hawking radiation from Kerr-(anti)de Sitter black holes by using gravitational anomaly method developed in gr-qc/0502074. We consider the general Kerr-(anti)de Sitter black holes in arbitrary $D$ dimensions with the maximal number [D/2] of independent rotating parameters. We find that the physics near the horizon can be described by an infinite collection of $(1+1)$-dimensional quantum fields coupled to a set of gauge fields with charges proportional to the azimuthal angular momentums $m_i$. With the requirement of anomaly cancellation and regularity at the horizon, the Hawking radiation is determined. | |
| dc.description | 12 pages; A typo in the abstract corrected; The version to be published | |
| dc.identifier | https://arxiv.org/abs/hep-th/0612261 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0612261 | |
| dc.identifier | Phys.Rev.D75:024041,2007 | |
| dc.identifier | doi:10.1103/PhysRevD.75.024041 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/194910 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Hawking Radiation from General Kerr-(anti)de Sitter Black Holes | |
| dc.type | text |