Higher dimensional Yang-Mills black holes in third order Lovelock gravity
| dc.creator | Mazharimousavi, S. Habib | |
| dc.creator | Halilsoy, M. | |
| dc.date | 2008-01-11 | |
| dc.date | 2008-06-13 | |
| dc.date.accessioned | 2026-07-07T11:39:51Z | |
| dc.date.available | 2026-07-07T11:39:51Z | |
| dc.description | By employing the higher (N\TEXTsymbol{>}5) dimensional version of the Wu-Yang Ansatz we obtain magnetically charged new black hole solutions in the Einstein-Yang-Mills-Lovelock (EYML) theory with second ($α_{2}$) and third ($α_{3}$)order parameters. These parameters, where $α_{2}$ is also known as the Gauss-Bonnet parameter, modify the horizons (and the resulting thermodynamical properties) of the black holes. It is shown also that asymptotically ($r\to \infty $), these parameters contribute to an effective cosmological constant -without cosmological constant- so that the solution behaves de-Sitter (Anti de-Sitter) like. | |
| dc.description | 14 pages, 3 figures, to appear in Phys. Lett. B | |
| dc.identifier | https://arxiv.org/abs/0801.1726 | |
| dc.identifier | http://arxiv.org/abs/0801.1726 | |
| dc.identifier | Phys.Lett.B665:125-130,2008 | |
| dc.identifier | doi:10.1016/j.physletb.2008.06.007 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/200071 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Higher dimensional Yang-Mills black holes in third order Lovelock gravity | |
| dc.type | text |