Classical Yang-Mills black hole hair in anti-de Sitter space
| dc.creator | Winstanley, Elizabeth | |
| dc.date | 2008-01-03 | |
| dc.date.accessioned | 2026-07-07T12:34:40Z | |
| dc.date.available | 2026-07-07T12:34:40Z | |
| dc.description | The properties of hairy black holes in Einstein-Yang-Mills (EYM) theory are reviewed, focusing on spherically symmetric solutions. In particular, in asymptotically anti-de Sitter space (adS) stable black hole hair is known to exist for su(2) EYM. We review recent work in which it is shown that stable hair also exists in su(N) EYM for arbitrary N, so that there is no upper limit on how much stable hair a black hole in adS can possess. | |
| dc.description | 41 pages, 14 figures. Based on the lecture given at the 4th Aegean Summer School | |
| dc.identifier | https://arxiv.org/abs/0801.0527 | |
| dc.identifier | http://arxiv.org/abs/0801.0527 | |
| dc.identifier | Lect.Notes Phys.769:49-87,2009 | |
| dc.identifier | doi:10.1007/978-3-540-88460-6_2 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/217516 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Classical Yang-Mills black hole hair in anti-de Sitter space | |
| dc.type | text |