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

dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, Mustafa
dc.date.accessioned2016-01-05T11:03:26Z
dc.date.available2016-01-05T11:03:26Z
dc.date.issued2014
dc.descriptionThe file in this item is the publisher version (published version) of the article.
dc.description.abstractThe 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.description.versionPublisher Version; (Publisher’s PDF as it appears in the Journal).
dc.identifier.citationS. 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.issn1434-6052 (Online)
dc.identifier.issn1434-6044 (Print)
dc.identifier.otherDOI: 10.1140/epjc/s10052-014-3073-2
dc.identifier.urihttps://hdl.handle.net/11129/1912
dc.language.isoen
dc.publisherThe European Physical Journal C, Springeren_US
dc.relation.ispartofseriesSpringer;Eur. Phys. J. C (2014) 74:3073
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.subjectgeneral relativityen_US
dc.subjectblack holesen_US
dc.titleCounterrotational effects on stability of 2+1-dimensional thin-shell wormholesen_US
dc.typeArticle

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