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 |
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dc.date.issued |
2011 |
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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 |
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dc.identifier.other |
DOI: 10.1103/PhysRevD.84.064032 |
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dc.identifier.uri |
http://hdl.handle.net/11129/1942 |
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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). |
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