Bertotti-Robinson thin-shell wormhole is physical but unstable

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dc.contributor.authorAmirabi, Z.
dc.date.accessioned2026-02-06T18:51:29Z
dc.date.issued2016
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractI construct a thin-shell wormhole in the spherically symmetric, static Bertotti-Robinson magnetic universe which is supported by normal matter in the sense that the energy conditions are all satisfied. Using the so called small velocity perturbation it is shown that this thin-shell wormhole is basically physical but unstable against radial perturbation.
dc.identifier.doi10.1140/epjp/i2016-16270-8
dc.identifier.issn2190-5444
dc.identifier.issue8
dc.identifier.scopus2-s2.0-84982861769
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjp/i2016-16270-8
dc.identifier.urihttps://hdl.handle.net/11129/15351
dc.identifier.volume131
dc.identifier.wosWOS:000397597100001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer Heidelberg
dc.relation.ispartofEuropean Physical Journal Plus
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectGeneral-Relativity
dc.subjectTraversable Wormholes
dc.subjectComputer Algebra
dc.subjectStability
dc.subjectFormalism
dc.subjectDimensions
dc.subjectSpacetimes
dc.subjectJunctions
dc.subjectEnergy
dc.subjectThroat
dc.titleBertotti-Robinson thin-shell wormhole is physical but unstable
dc.typeArticle

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