Stability of spherically symmetric timelike thin-shells in general relativity with a variable equation-of-state

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dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, M.
dc.contributor.authorAmen, S. N. Hamad
dc.date.accessioned2026-02-06T18:51:36Z
dc.date.issued2017
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWe study spherically symmetric timelike thin-shells in 3+1-dimensional bulk spacetime with a variable equation-of-state for the fluid presented on the shell. In such a fluid, the angular pressure p is a function of both surface energy density sigma and the radius R of the thin-shell. Explicit cases of the thin shells connecting two nonidentical cloud of strings spacetimes and a flat Minkowski spacetime to the Schwarzschild metric are investigated.
dc.identifier.doi10.1142/S0218271817501589
dc.identifier.issn0218-2718
dc.identifier.issn1793-6594
dc.identifier.issue14
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.scopus2-s2.0-85025165444
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1142/S0218271817501589
dc.identifier.urihttps://hdl.handle.net/11129/15441
dc.identifier.volume26
dc.identifier.wosWOS:000417162100007
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Modern Physics D
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectThin-shell
dc.subjectspherically symmetric
dc.subjectstability
dc.subjectvariable equation-of-state
dc.titleStability of spherically symmetric timelike thin-shells in general relativity with a variable equation-of-state
dc.typeArticle

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