On the energy-momentum problem in static Einstein universe

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dc.contributor.authorAygun, S.
dc.contributor.authorTarhan, I.
dc.contributor.authorBaysal, H.
dc.date.accessioned2025-01-27T20:54:09Z
dc.date.available2025-01-27T20:54:09Z
dc.date.issued2007
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThe energy-momentum distributions of Einstein's simplest static geometrical model for an isotropic and homogeneous universe are evaluated. For this purpose, Einstein, Bergmann-Thomson, Landau-Lifshitz (LL), Moller and Papapetrou energy-momentum complexes are used in general relativity. While Einstein and Bergmann-Thomson complexes give exactly the same results, LL and Papapetrou energy-momentum complexes do not provide the same energy densities. The Moller energy-momentum density is found to be zero everywhere in Einstein's universe. Also, several spacetimes are the limiting cases considered here.
dc.identifier.doi10.1088/0256-307X/24/2/015
dc.identifier.endpage358
dc.identifier.issn0256-307X
dc.identifier.issn1741-3540
dc.identifier.issue2
dc.identifier.scopus2-s2.0-34247191239
dc.identifier.scopusqualityQ1
dc.identifier.startpage355
dc.identifier.urihttps://doi.org/10.1088/0256-307X/24/2/015
dc.identifier.urihttps://hdl.handle.net/20.500.12428/25993
dc.identifier.volume24
dc.identifier.wosWOS:000244116400015
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIop Publishing Ltd
dc.relation.ispartofChinese Physics Letters
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjectRadiating Charged-Particle
dc.subjectBlack-Hole
dc.subjectGeneral Theory
dc.subjectTetrad Theory
dc.subjectLocalization
dc.subjectDistributions
dc.subjectSpacetime
dc.subjectMass
dc.titleOn the energy-momentum problem in static Einstein universe
dc.typeArticle

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