dc.contributor.author |
Mazharimousavi, S. Habib |
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dc.contributor.author |
Halilsoy, Mustafa |
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dc.contributor.author |
Amirabi, Zahra |
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dc.date.accessioned |
2016-01-20T13:51:33Z |
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dc.date.available |
2016-01-20T13:51:33Z |
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dc.date.issued |
2009 |
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dc.identifier.citation |
S. Habib Mazharimousavi, Mustafa Halilsoy and Zahra Amirabi, General Relativity and Gravitation 28 (2009) 261: arXiv:0802.3990"N-Dimensional non-abelian dilatonic,stable black holes and their Born-Infeld extension". |
en_US |
dc.identifier.issn |
1572-9532 (online) |
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dc.identifier.issn |
0001-7701 (online) |
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dc.identifier.other |
DOI: 10.1007/s10714-009-0835-5 |
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dc.identifier.uri |
http://dx.doi.org/10.1007/s10714-009-0835-5 |
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dc.identifier.uri |
http://hdl.handle.net/11129/2032 |
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dc.description |
The file in this item is the post-print version of the article (author’s copy; author’s final manuscript, accepted for publication after peer-review process). Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI (with DOI: 10.1007/s10714-009-0835-5) and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication. |
en_US |
dc.description.abstract |
We find large classes of non-asymptotically flat Einstein-Yang-Mills-Dilaton (EYMD) and Einstein-Yang-Mills-Born-Infeld-Dilaton (EYMBID) black holes in N-dimensional spherically symmetric spacetime expressed in terms of the quasilocal mass. Extension of the dilatonic YM solution to N-dimensions has been possible by employing the generalized Wu-Yang ansatz. Another metric ansatz, which aided in finding exact solutions is the functional dependence of the radius function on the dilaton field. These classes of black holes are stable against linear radial perturbations. In the limit of vanishing dilaton we obtain Bertotti-Robinson (BR) type metrics with the topology of AdS2×SN−2. Since connection can be established between dilaton and a scalar field of Brans-Dicke (BD) type we obtain black hole solutions also in the Brans-Dicke-Yang-Mills (BDYM) theory as well. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.publisher |
General Relativity and Gravitation, Springer |
en_US |
dc.relation.ispartofseries |
;Gen Rel.Grav.42:261-280,2010 |
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dc.subject |
gravity |
en_US |
dc.subject |
general relativity |
en_US |
dc.subject |
non-abelian dilatonic |
en_US |
dc.subject |
black holes |
en_US |
dc.subject |
Born-Infeld |
en_US |
dc.title |
N-Dimensional non-abelian dilatonic, stable black holes and their Born-Infeld extension |
en_US |
dc.type |
Article |
en_US |
dc.description.version |
Post-Print Author Version (Final Author Manuscript, accepted for publication, after peer-review process). |
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