Rotating Thin-Shell Wormhole

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dc.contributor.author	Övgün, Ali
dc.date.accessioned	2016-11-08T19:28:25Z
dc.date.available	2016-11-08T19:28:25Z
dc.date.issued	2016-11-08
dc.identifier.issn	2190-5444 (print)
dc.identifier.issn	2190-5444 (online)
dc.identifier.uri	https://arxiv.org/abs/1604.08477
dc.identifier.uri	http://dx.doi.org/10.1140/epjp/i2016-16389-6
dc.identifier.uri	http://hdl.handle.net/11129/3066
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 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 construct a rotating thin-shell wormhole using a Myers-Perry black hole in five dimensions, using the Darmois-Israel junction conditions. The stability of the wormhole is analyzed under perturbations. We find that exotic matter is required at the throat of the wormhole to keep it stable. Our analysis shows that stability of the rotating thin-shell wormhole is possible if suitable parameter values are chosen.	en_US
dc.language.iso	eng	en_US
dc.publisher	SpringerLink	en_US
dc.relation.isversionof	10.1140/epjp/i2016-16389-6	en_US
dc.rights	info:eu-repo/semantics/openAccess	en_US
dc.subject	black hole	en_US
dc.subject	wormhole	en_US
dc.subject	thin-shell	en_US
dc.subject	rotating black holes	en_US
dc.subject	Myers-Perry	en_US
dc.subject	Darmois-Israel junction conditions	en_US
dc.title	Rotating Thin-Shell Wormhole	en_US
dc.type	article	en_US
dc.relation.journal	The European Physical Journal - Plus (EPJ Plus)	en_US
dc.contributor.department	Eastern Mediterranean University, Faculty of Arts and Sciences, Department of Physics	en_US
dc.identifier.volume	131	en_US
dc.identifier.issue	389	en_US