Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes

dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.date.accessioned	2016-01-05T11:03:26Z
dc.date.available	2016-01-05T11:03:26Z
dc.date.issued	2014
dc.identifier.citation	S. HabibMazharimousavi and M. Halilsoy, arXiv:1407.4673 “Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes” Eur. Phys. J. C 74, 3073 (2014).	en_US
dc.identifier.issn	1434-6052 (Online)
dc.identifier.issn	1434-6044 (Print)
dc.identifier.other	DOI: 10.1140/epjc/s10052-014-3073-2
dc.identifier.uri	http://hdl.handle.net/11129/1912
dc.description	The file in this item is the publisher version (published version) of the article.
dc.description.abstract	The role of angular momentum in a 2+1-dimensional rotating thin-shell wormhole (TSW) is considered. Particular emphasis is made on stability when the shells (rings) are counterrotating. We find that counter-rotating halves make the TSW supported by the equation of state of a linear gas more stable. Under a small velocity dependent perturbation, however, it becomes unstable.	en_US
dc.language.iso	en_US	en_US
dc.publisher	The European Physical Journal C, Springer	en_US
dc.relation.ispartofseries	Springer;Eur. Phys. J. C (2014) 74:3073
dc.subject	general relativity	en_US
dc.subject	black holes	en_US
dc.title	Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version; (Publisher’s PDF as it appears in the Journal).