Cylindrically-symmetric and inhomogeneous cosmological models with viscous fluid

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dc.contributor.authorKilinc, CB
dc.contributor.authorYavuz, I
dc.date.accessioned2025-01-27T20:27:28Z
dc.date.available2025-01-27T20:27:28Z
dc.date.issued1997
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this paper, the Einstein field equations have been solved for cylindrically symmetric and inhomogeneous cosmological models with viscous fluid. Various physical and geometrical properties of the models are also discussed.
dc.identifier.doi10.1023/A:1000351212513
dc.identifier.endpage142
dc.identifier.issn0004-640X
dc.identifier.issue1
dc.identifier.scopus2-s2.0-0040651688
dc.identifier.scopusqualityQ2
dc.identifier.startpage131
dc.identifier.urihttps://doi.org/10.1023/A:1000351212513
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22700
dc.identifier.volume249
dc.identifier.wosWOS:A1997YB89700010
dc.identifier.wosqualityQ4
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherKluwer Academic Publ
dc.relation.ispartofAstrophysics and Space Science
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectElectromagnetic-Field
dc.subjectIntrinsic Symmetries
dc.titleCylindrically-symmetric and inhomogeneous cosmological models with viscous fluid
dc.typeArticle

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