| dc.contributor.author | Mazharimousavi, S. Habib | |
| dc.contributor.author | Halilsoy, Mustafa | |
| dc.date.accessioned | 2016-01-07T14:21:59Z | |
| dc.date.available | 2016-01-07T14:21:59Z | |
| dc.date.issued | 2011 | |
| dc.identifier.citation | S. Habib Mazharimousavi and M. Halilsoy (2011) arXiv:1105.3659 "Black hole solutions in f(R) gravity coupled with non-linear Yang-Mills eld", Phys. Rev. D 84 (2011) 064032. | en_US |
| dc.identifier.issn | 1550-7998 | |
| dc.identifier.other | DOI: 10.1103/PhysRevD.84.064032 | |
| dc.identifier.uri | http://hdl.handle.net/11129/1942 | |
| dc.description | The file in this item is the publisher version (published version) of the article. | en_US |
| dc.description.abstract | It is shown that in the static, spherically symmetric spacetime the problem of metric f(R) gravity coupled with non-linear Yang-Mills (YM) field constructed from the Wu-Yang ansatz as source, can be solved in all dimensions. By non-linearity it is meant that the YM Lagrangian depends arbitrarily on its invariant. A particular form is considered to be in the power-law form with limit of the standard YM theory. The formalism admits black hole solutions with single or double horizons in which f(R) can be obtained, in general numerically. In 6-dimensional case we obtain an exact solution given by f(R)=\surdR gravity that couples with the YM field in a consistent manner. | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | Physical Review D, American Physical Society (APS) | en_US |
| dc.relation.ispartofseries | ;Phys. Rev. D 84, 064032 (2011) | |
| dc.subject | general relativity | en_US |
| dc.subject | black holes | en_US |
| dc.title | Black hole solutions in f(R) gravity coupled with non-linear Yang-Mills field | en_US |
| dc.type | Article | en_US |
| dc.description.version | Publisher Version (Published Version). |