Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity

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dc.contributor.author	Amirabi, Zahra
dc.contributor.author	Halilsoy, Mustafa
dc.contributor.author	Mazharimousavi, S. Habib
dc.date.accessioned	2016-01-15T13:34:41Z
dc.date.available	2016-01-15T13:34:41Z
dc.date.issued	2013
dc.identifier.citation	Z. Amirabi, M. Halilsoy and S. HabibMazharimousavi, arXiv:1103.3019 "Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity". Phys. Rev. D 88, 124023 (2013).	en_US
dc.identifier.issn	1550-7998
dc.identifier.other	DOI: 10.1103/PhysRevD.88.124023
dc.identifier.uri	http://hdl.handle.net/11129/1989
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	We study the stability of thin-shell wormholes in Einstein-Maxwell-Gauss-Bonnet gravity. The equation of state of the thin shell wormhole is considered first to obey a generalized Chaplygin gas and then we generalize it to an arbitrary state function which covers all known cases studied so far. In particular we study the modified Chaplygin gas and give an assessment for a general parotropic fluid. Our study is in d-dimensions and with numerical analysis in d=5 we show the effect of the GB parameter in the stability of thin-shell wormholes against the radial perturbations.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Physical Review D, American Physical Society (APS)	en_US
dc.relation.ispartofseries	;Phys. Rev. D 88, 124023 (2013)
dc.subject	thin-shell wormholes	en_US
dc.subject	general relativity	en_US
dc.subject	wormholes	en_US
dc.subject	gravity	en_US
dc.subject	Einstein-Maxwell-Gauss-Bonnet gravity	en_US
dc.title	Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).