Special Standard Static Space-Times

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dc.authorscopusid8704767500
dc.authorscopusid7005860624
dc.authorwosidUnal, Bulent/I-7795-2012
dc.contributor.authorDobarro, F
dc.contributor.authorÜnal, B
dc.contributor.otherDepartment of Modern Languages
dc.date.accessioned2024-07-05T15:09:23Z
dc.date.available2024-07-05T15:09:23Z
dc.date.issued2004
dc.departmentAtılım Universityen_US
dc.department-tempUniv Trieste, Dipartimento Matemat & Informat, I-34127 Trieste, Italy; Atilim Univ, Dept Math, TR-06836 Ankara, Turkeyen_US
dc.description.abstractEssentially, some conditions for the Riemannian factor and the warping function of a standard static space-time are obtained in order to guarantee that no nontrivial warping function on the Riemannian factor can make the standard static space-time Einstein. (C) 2004 Elsevier Ltd. All rights reserved.en_US
dc.identifier.citationcount17
dc.identifier.doi10.1016/j.na.2004.07.035
dc.identifier.endpage770en_US
dc.identifier.issn0362-546X
dc.identifier.issn1873-5215
dc.identifier.issue5en_US
dc.identifier.scopus2-s2.0-7244251445
dc.identifier.scopusqualityQ2
dc.identifier.startpage759en_US
dc.identifier.urihttps://doi.org/10.1016/j.na.2004.07.035
dc.identifier.urihttps://hdl.handle.net/20.500.14411/1159
dc.identifier.volume59en_US
dc.identifier.wosWOS:000225022900010
dc.identifier.wosqualityQ1
dc.institutionauthorÜnal, Bernis
dc.language.isoenen_US
dc.publisherPergamon-elsevier Science Ltden_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.scopus.citedbyCount20
dc.subjectspace-timeen_US
dc.subjectwarped producten_US
dc.subjectEinstein manifolden_US
dc.subjectRicci-flaten_US
dc.subjectscalar curvatureen_US
dc.titleSpecial Standard Static Space-Timesen_US
dc.typeArticleen_US
dc.wos.citedbyCount18
dspace.entity.typePublication
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relation.isOrgUnitOfPublication31554256-c410-403f-9195-717f892be9f7
relation.isOrgUnitOfPublication.latestForDiscovery31554256-c410-403f-9195-717f892be9f7

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