Conditions for nonexistence of static or stationary, Einstein-Maxwell, non-inheriting black-holes
| dc.creator | Tod, Paul | |
| dc.date | 2006-11-05 | |
| dc.date.accessioned | 2026-07-07T10:24:39Z | |
| dc.date.available | 2026-07-07T10:24:39Z | |
| dc.description | We consider asymptotically-flat, static and stationary solutions of the Einstein equations representing Einstein-Maxwell space-times in which the Maxwell field is not constant along the Killing vector defining stationarity, so that the symmetry of the space-time is not inherited by the electromagnetic field. We find that static degenerate black hole solutions are not possible and, subject to stronger assumptions, nor are static, non-degenerate or stationary black holes. We describe the possibilities if the stronger assumptions are relaxed. | |
| dc.description | 19 pages, to appear in GERG | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0611035 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0611035 | |
| dc.identifier | Gen.Rel.Grav.39:111-127,2007 | |
| dc.identifier | doi:10.1007/s10714-006-0363-5 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/176262 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Conditions for nonexistence of static or stationary, Einstein-Maxwell, non-inheriting black-holes | |
| dc.type | text |