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dc.contributor.authorTiwari, Rishi Kumar
dc.contributor.authorMishra, Sateesh Kumar
dc.contributor.authorSOFUOĞLU, Değer
dc.date.accessioned2021-02-28T14:35:06Z
dc.date.available2021-02-28T14:35:06Z
dc.identifier.citationTiwari R. K. , SOFUOĞLU D., Mishra S. K. , "Accelerating universe with varying A in f(R, T) theory of gravity", NEW ASTRONOMY, cilt.83, 2021
dc.identifier.issn1384-1076
dc.identifier.othervv_1032021
dc.identifier.otherav_58fd1757-0662-4d5a-93ff-5d4eab79aa13
dc.identifier.urihttp://hdl.handle.net/20.500.12627/1522
dc.identifier.urihttps://doi.org/10.1016/j.newast.2020.101476
dc.identifier.urihttps://doi.org/10.1016/j.newast.2020.101476
dc.description.abstractIn this paper we have investigated Bianchi Type-I cosmological model with varying cosmological constant A in f (R, T) theory of gravity. In order to obtain an exact solution of the field equations, we have used a special law of Hubble parameter proposed by Banerjee and Das (Gen Relat Gravit 37 (2005) 1695-1703), which leads to a time dependent deceleration parameter. We have discussed the physical and kinematical properties of the model in detail. The statefinder diagnostic parameters have also been considered. It has been shown that our universe model is consistent with the recent observations and approaches the ACDM model at late times.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectUzay bilimi
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleAccelerating universe with varying A in f(R, T) theory of gravity
dc.typeMakale
dc.relation.journalNEW ASTRONOMY
dc.contributor.department, Govt. Model Science College , Mathematics
dc.identifier.volume83
dc.contributor.firstauthorID2358686


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