Energy distributions in Szekeres type I and II space-times

dc.contributor.authorAygun, Sezgin
dc.contributor.authorAygun, Melis
dc.contributor.authorTarhan, Ismail
dc.date.accessioned2025-01-27T20:24:26Z
dc.date.available2025-01-27T20:24:26Z
dc.date.issued2006
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this study, in context of general relativity we consider Einstein, Bergmann-Thomson, Moller and Landau-Lifshitz energy-momentum definitions and we compute the total energy distribution (due to matter and fields including gravitation) of the universe based on Szekeres class I and class II space-times. We show that Einstein and Bergmann-Thomson definitions of the energy-momentum complexes give the same results, while Moller's and Landau-Lifshitz's energy-momentum definition does not provide same results for Szekeres class II space. The definitions of Einstein, Bergmann-Thomson and Moller definitions of the energy-momentum complexes give similar results in Szekeres class I space-time.
dc.identifier.endpage2793
dc.identifier.issn0587-4254
dc.identifier.issue10
dc.identifier.scopus2-s2.0-33750027908
dc.identifier.scopusqualityQ3
dc.identifier.startpage2781
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22224
dc.identifier.volume37
dc.identifier.wosWOS:000241402900004
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherPolish Acad Sciences Inst Physics
dc.relation.ispartofActa Physica Polonica B
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectCylindrical Gravitational-Waves
dc.subjectGeneral-Relativity
dc.subjectCosmological Models
dc.subjectAngular-Momentum
dc.subjectUniverse
dc.subjectEinstein
dc.subjectLocalization
dc.subjectGravity
dc.subjectMass
dc.titleEnergy distributions in Szekeres type I and II space-times
dc.typeArticle

Dosyalar