Rigidly rotating strange quark stars

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dc.contributor.authorYilmaz, I
dc.contributor.authorBaysal, H
dc.date.accessioned2025-01-27T20:34:35Z
dc.date.available2025-01-27T20:34:35Z
dc.date.issued2005
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this article, we study rotating strange quark stars in the context of general relativity. For this purpose we consider perfect fluid model composed of strange quark matter with electromagnetic field in the Godel Universe which has rigid rotation. We solve Einstein's field equations by using equation of state for strange quark matter. Also, we discuss the features of obtained solutions.
dc.identifier.doi10.1142/S0218271805006158
dc.identifier.endpage705
dc.identifier.issn0218-2718
dc.identifier.issn1793-6594
dc.identifier.issue3-4
dc.identifier.scopus2-s2.0-21244446662
dc.identifier.scopusqualityQ1
dc.identifier.startpage697
dc.identifier.urihttps://doi.org/10.1142/S0218271805006158
dc.identifier.urihttps://hdl.handle.net/20.500.12428/23369
dc.identifier.volume14
dc.identifier.wosWOS:000229550300016
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.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjectstrange quark star
dc.subjectGodel universe
dc.subjectelectromagnetic field
dc.titleRigidly rotating strange quark stars
dc.typeArticle

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