Rotating Black Holes in Higher Dimensional Einstein-Maxwell Gravity
| dc.creator | Aliev, A. N. | |
| dc.date | 2006-04-27 | |
| dc.date | 2006-07-13 | |
| dc.date.accessioned | 2026-07-07T10:46:31Z | |
| dc.date.available | 2026-07-07T10:46:31Z | |
| dc.description | The strategy of obtaining the familiar Kerr-Newman solution in general relativity is based on either using the metric ansatz in the Kerr-Schild form, or applying the method of complex coordinate transformation to a non-rotating charged black hole. In practice, this amounts to an appropriate re-scaling of the mass parameter in the metric of uncharged black holes. Using a similar approach, we assume a special metric ansatz in N+1 dimensions and present a new analytic solution to the Einstein-Maxwell system of equations. It describes rotating charged black holes with a single angular momentum in the limit of slow rotation. We also give the metric for a slowly rotating charged black hole with two independent angular momenta in five dimensions. We compute the gyromagnetic ratio of these black holes which corresponds to the value g=N-1. | |
| dc.description | 19 pages, minor changes, typos corrected | |
| dc.identifier | https://arxiv.org/abs/hep-th/0604207 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0604207 | |
| dc.identifier | Phys.Rev.D74:024011,2006 | |
| dc.identifier | doi:10.1103/PhysRevD.74.024011 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183258 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Rotating Black Holes in Higher Dimensional Einstein-Maxwell Gravity | |
| dc.type | text |