Thin-shells and thin-shell wormholes in new massive gravity

dc.contributor.authorForghani, S. Danial
dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, M.
dc.date.accessioned2026-02-06T18:51:19Z
dc.date.issued2019
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWithin 2 + 1-dimensional cosmological new massive gravity, we consider thin-shell and thin-shell wormhole construction. For this, we introduce first, the junction conditions apt for the fourth order terms in the action of the theory. Then, by employing some specific static solutions in new massive gravity, we study the characteristics of associated thin-shells and thin-shell wormholes. Our finding suggests that, firstly, there cannot exist any thin-shells regarding our chosen solutions of cosmological new massive gravity, and secondly, the constructed thin-shell wormhole does not need to be symmetric. More importantly, the thin-shell wormhole, if ever forms, possesses null energy density and null angular pressure on its throat which are preferable to their negative-valued counterparts.
dc.identifier.doi10.1140/epjc/s10052-019-6964-4
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.issue6
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.orcid0000-0002-6170-826X
dc.identifier.scopus2-s2.0-85068756423
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-019-6964-4
dc.identifier.urihttps://hdl.handle.net/11129/15288
dc.identifier.volume79
dc.identifier.wosWOS:000469426600003
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofEuropean Physical Journal C
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectLinearized Stability
dc.titleThin-shells and thin-shell wormholes in new massive gravity
dc.typeArticle

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