Stability of generic cylindrical thin shell wormholes

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dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.contributor.author	Amirabi, Zahra
dc.date.accessioned	2016-01-05T12:26:18Z
dc.date.available	2016-01-05T12:26:18Z
dc.date.issued	2014
dc.identifier.citation	S. Habib Mazharimousavi, M. Halilsoy and Z. Amirabi, arXiv:1403.2861 "Stability of generic cylindrical thin shell wormholes". Physical Review D 89, 084003 (2014).	en_US
dc.identifier.issn	1550-7998
dc.identifier.other	DOI: 10.1103/PhysRevD.89.084003
dc.identifier.uri	http://hdl.handle.net/11129/1916
dc.description	The file in this item is the publisher version (published version) of the article.
dc.description.abstract	We revisit the stability analysis of cylindrical thin shell wormholes which have been studied in literature so far. Our approach is more systematic and in parallel to the method which is used in spherically symmetric thin shell wormholes. The stability condition is summarized as the positivity of the second derivative of an effective potential at the equilibrium radius, i.e. V′′(a0)>0. This may serve as the master equation in all stability problems for the cylindrical thin-shell wormholes.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Physical Review D, American Physical Society (APS)	en_US
dc.relation.ispartofseries	;Physical Review D 89, 084003 (2014)
dc.subject	general relativity	en_US
dc.subject	black holes	en_US
dc.title	Stability of generic cylindrical thin shell wormholes	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version; (Publisher’s PDF as it appears in the Journal).