Schwarzschild-Levi-Civita black hole

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dc.contributor.authorMazharimousavi, S. Habib
dc.date.accessioned2026-02-06T18:40:25Z
dc.date.issued2025
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractInspired by the geometry of the Ernst black hole which interpolates the static spherically symmetric Schwarzschild black hole and the static axially symmetric magnetic Melvin spacetime, in this paper, we aim to present a solution to Einstein's field equation in vacuum to interpolate the Schwarzschild black hole and the Levi-Civita spacetime. Hence, we shall call the solution the Schwarzschild-Levi-Civita black hole. Effectively the solution is a two- parameter non-asymptotically flat black hole that is static, axially symmetric, and singular in its axis of symmetry.
dc.identifier.doi10.1016/j.physletb.2024.139234
dc.identifier.issn0370-2693
dc.identifier.issn1873-2445
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.scopus2-s2.0-85213849799
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1016/j.physletb.2024.139234
dc.identifier.urihttps://hdl.handle.net/11129/13291
dc.identifier.volume861
dc.identifier.wosWOS:001398249400001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier
dc.relation.ispartofPhysics Letters B
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectSchwarszchild black hole
dc.subjectLevi-Civita metric
dc.subjectVacuum black hole
dc.subjectExact solution
dc.titleSchwarzschild-Levi-Civita black hole
dc.typeArticle

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