Relativistic Bose-Einstein condensates thin-shell wormholes

dc.contributor.authorRicharte, M. G.
dc.contributor.authorSalako, I. G.
dc.contributor.authorMorais Graca, J. P.
dc.contributor.authorMoradpour, H.
dc.contributor.authorOvgun, Ali
dc.date.accessioned2026-02-06T18:49:02Z
dc.date.issued2017
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWe construct traversable thin-shell wormholes which are asymptotically Ads/dS applying the cut and paste procedure for the case of an acoustic metric created by a relativistic Bose-Einstein condensate. We examine several definitions of the flare-out condition along with the violation or not of the energy conditions for such relativistic geometries. Under reasonable assumptions about the equation of state of the matter located at the shell, we concentrate on the mechanical stability of wormholes under radial perturbation preserving the original spherical symmetry. To do so, we consider linearized perturbations around static solutions. We obtain that dS acoustic wormholes remain stable under radial perturbations as long as they have small radius; such wormholes with finite radius do not violate the strong/null energy condition. Besides, we show that stable Ads wormhole satisfy some of the energy conditions whereas unstable Ads wormhole with large radii violate them.
dc.description.sponsorshipConselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)- Brazil; Research Institute for Astronomy & Astrophysics of Maragha (RIAAM) [1/4165-1]; Chilean FONDECYT [3170035]
dc.description.sponsorshipM. G.R and J. P. M.G are supported by Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)- Brazil. The work of H. Moradpour has been supported financially by Research Institute for Astronomy & Astrophysics of Maragha (RIAAM) under project No. 1/4165-1. The work of A.O is supported by the Chilean FONDECYT Grant No. 3170035.
dc.identifier.doi10.1103/PhysRevD.96.084022
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.issue8
dc.identifier.orcid0000-0001-5705-6185
dc.identifier.orcid0000-0003-0941-8422
dc.identifier.orcid0000-0002-9889-342X
dc.identifier.orcid0000-0002-2721-280X
dc.identifier.scopus2-s2.0-85032979698
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.96.084022
dc.identifier.urihttps://hdl.handle.net/11129/14711
dc.identifier.volume96
dc.identifier.wosWOS:000412702600003
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Physical Soc
dc.relation.ispartofPhysical Review D
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectWeak Energy Condition
dc.subjectCharged Black-Holes
dc.subjectTraversable Wormholes
dc.subjectGeneral-Relativity
dc.subjectLinearized Stability
dc.subjectMaxwell Theory
dc.subjectTime Machines
dc.subjectGravity
dc.subjectFormalism
dc.titleRelativistic Bose-Einstein condensates thin-shell wormholes
dc.typeArticle

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