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dc.contributor.authorSofuoglu, DEĞER
dc.date.accessioned2021-03-05T07:37:47Z
dc.date.available2021-03-05T07:37:47Z
dc.date.issued2016
dc.identifier.citationSofuoglu D., "Rotating and expanding Bianchi type-IX model in f (R, T) theory of gravity", ASTROPHYSICS AND SPACE SCIENCE, cilt.361, 2016
dc.identifier.issn0004-640X
dc.identifier.othervv_1032021
dc.identifier.otherav_94cf6aa8-57d7-4fe5-9a71-01c39cd91879
dc.identifier.urihttp://hdl.handle.net/20.500.12627/100223
dc.identifier.urihttps://doi.org/10.1007/s10509-015-2593-z
dc.description.abstractThe spatially homogeneous shear-free, rotating and expanding Bianchi type-IX universe has been considered in the presence of perfect fluid in f (R, T) theory of gravity. The exact solution of the field equations has been obtained and the functional form of f (R, T) = R + 2f (T) gravity has been reconstructed. The existence of such a solution suggests that the general relativistic shear-free perfect fluid conjecture which claims that a shear-free perfect fluid cannot rotate and expand at the same time, is not valid in this modified theory.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleRotating and expanding Bianchi type-IX model in f (R, T) theory of gravity
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.departmentİstanbul Üniversitesi , ,
dc.identifier.volume361
dc.identifier.issue1
dc.contributor.firstauthorID227340


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