Note on the Levi-Civita metric

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dc.contributor.authorHalilsoy, M.
dc.contributor.authorMazharimousavi, S. Habib
dc.date.accessioned2026-02-06T18:51:43Z
dc.date.issued2022
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractBy introducing a new coordinate condition we divide the cylindrical spacetime of Levi-Civita (LC) into a sourceful inner (rho < rho(0) = const.) and vacuum outer (rho >= rho(0)) regions. The emergent fluid with zero radial pressure confined to the finely-tuned inner region serves to make the spacetime regular in a natural way. At rho = 0 the LC spacetime becomes 'Cartesian flat' so that no deficit angle arises.
dc.identifier.doi10.1142/S0219887822501663
dc.identifier.issn0219-8878
dc.identifier.issn1793-6977
dc.identifier.issue11
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.scopus2-s2.0-85132970237
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1142/S0219887822501663
dc.identifier.urihttps://hdl.handle.net/11129/15481
dc.identifier.volume19
dc.identifier.wosWOS:000848629300002
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Geometric Methods in Modern Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectLevi-Civita metric
dc.subjectregular spacetime
dc.subjectexact solution
dc.titleNote on the Levi-Civita metric
dc.typeArticle

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