The null circular geodesic outside the spherically symmetric asymptotically flat hairy black hole is not stable

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dc.contributor.authorMazharimousavi, S. Habib
dc.date.accessioned2026-02-06T18:51:21Z
dc.date.issued2024
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn this study, we explicitly prove that the null circular orbit outside the spherically symmetric asymptotically flat hairy black hole is not stable. Although, if there is more than one external light ring at least one of them is stable. The existence of such geodesics has been proved in the recent work of Hod as well as Peng whereas its stability was left uncommented.
dc.identifier.doi10.1140/epjc/s10052-024-12447-9
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.issue1
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.scopus2-s2.0-85183017322
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-024-12447-9
dc.identifier.urihttps://hdl.handle.net/11129/15317
dc.identifier.volume84
dc.identifier.wosWOS:001150392100001
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.titleThe null circular geodesic outside the spherically symmetric asymptotically flat hairy black hole is not stable
dc.typeArticle

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