EMU I-REP >
08 Faculty of Arts and Sciences >
Department of Physics >
PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics >
Please use this identifier to cite or link to this item:
http://hdl.handle.net/11129/2032
|
Title: | N-Dimensional non-abelian dilatonic, stable black holes and their Born-Infeld extension |
Authors: | Mazharimousavi, S. Habib Halilsoy, Mustafa Amirabi, Zahra |
Keywords: | gravity general relativity non-abelian dilatonic black holes Born-Infeld |
Issue Date: | 2009 |
Publisher: | General Relativity and Gravitation, Springer |
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". |
Series/Report no.: | ;Gen Rel.Grav.42:261-280,2010 |
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. |
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. |
URI: | http://dx.doi.org/10.1007/s10714-009-0835-5 http://hdl.handle.net/11129/2032 |
ISSN: | 1572-9532 (online) 0001-7701 (online) |
Appears in Collections: | PHY – Journal Articles: Publisher & Author Versions (Post-Print Author Versions) – Physics
|
This item is protected by original copyright
|
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.
|