Higher dimensional thin-shell wormholes in Einstein-Yang-Mills-Gauss-Bonnet gravity

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dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.contributor.author	Amirabi, Zahra
dc.date.accessioned	2016-01-19T12:47:28Z
dc.date.available	2016-01-19T12:47:28Z
dc.date.issued	2011
dc.identifier.citation	S. Habib Mazharimousavi, M. Halilsoy and Z. Amirabi, Class. Quant. Grav. 28 (2011) 025004, arXiv:0082365 "Higher dimensional thin-shell wormholes in Einstein-Yang-Mills-Gauss-Bonnet gravity".	en_US
dc.identifier.issn	ISSN: 1361-6382 (online)
dc.identifier.issn	ISSN: 0264-9381 (print)
dc.identifier.other	DOI: 10.1088/0264-9381/28/2/025004
dc.identifier.uri	http://dx.doi.org/10.1088/0264-9381/28/2/025004
dc.identifier.uri	http://hdl.handle.net/11129/2008
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: 10.1088/0264-9381/28/2/025004) 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 present thin-shell wormhole solutions in Einstein-Yang-Mills-Gauss-Bonnet (EYMGB) theory in higher dimensions d\geq5. Exact black hole solutions are employed for this purpose where the radius of thin-shell lies outside the event horizon. For some reasons the cases d=5 and d>5 are treated separately. The surface energy-momentum of the thin-shell creates surface pressures to resist against collapse and rendering stable wormholes possible. We test the stability of the wormholes against spherical perturbations through a linear energy-pressure relation and plot stability regions. Apart from this restricted stability we investigate the possibility of normal (i.e. non-exotic) matter which satisfies the energy conditions. For negative values of the Gauss-Bonnet (GB) parameter we obtain such physical wormholes.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Classical and Quantum Gravity, Institute of Physics (IOP) Publishing: Hybrid Open Access - Green Policies in RoMEO	en_US
dc.relation.ispartofseries	IOP SCIENCE;Class.Quant.Grav.28:025004,2011
dc.subject	gravity	en_US
dc.subject	general relativity	en_US
dc.subject	wormholes	en_US
dc.subject	thin-shell wormholes	en_US
dc.subject	Einstein-Yang-Mills-Gauss-Bonnet gravity	en_US
dc.title	Higher dimensional thin-shell wormholes in Einstein-Yang-Mills-Gauss-Bonnet gravity	en_US
dc.type	Article	en_US