Scalar Field Cosmology in f(R,T) Gravity with Λ

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dc.authoridAygün, Sezgin / 0000-0002-2969-4195
dc.authoridAktaş, Can / 0000-0002-0603-7862
dc.contributor.authorAygün, Sezgin
dc.contributor.authorAktaş, Can
dc.contributor.authorSahoo, Pradyumn Kumar
dc.contributor.authorBishi, Binaya K.
dc.date.accessioned2025-01-27T18:56:06Z
dc.date.available2025-01-27T18:56:06Z
dc.date.issued2018
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractWe study the behavior of cosmological parameters, massive and massless scalar fields (normal or phantom) with a scalar potential in f(R, T) theory of gravity for a flat Friedmann-Robertson-Walker (FRW) universe. To get exact solutions to the modified field equations, we use the f(R, T) = R + 2f(T) model by Harko et al. (T. Harko et al., Phys. Rev. D 84, 024020 (2011)), where R is the Ricci scalar and T is the trace of the energy momentum tensor. Our cosmological parameter solutions agree with the recent observational data. Finally, we discuss our results with various graphics. © 2018, Pleiades Publishing, Ltd.
dc.description.sponsorshipÇanakkale Onsekiz Mart Üniversitesi, ÇOMÜ, (FBA-2017-1123)
dc.identifier.doi10.1134/S0202289318030039
dc.identifier.endpage307
dc.identifier.issn0202-2893
dc.identifier.issue3
dc.identifier.scopus2-s2.0-85052249042
dc.identifier.scopusqualityQ3
dc.identifier.startpage302
dc.identifier.urihttps://doi.org/10.1134/S0202289318030039
dc.identifier.urihttps://hdl.handle.net/20.500.12428/12858
dc.identifier.volume24
dc.identifier.wosWOS:000442627300012
dc.identifier.wosqualityQ4
dc.indekslendigikaynakScopus
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherPleiades Publishing
dc.relation.ispartofGravitation and Cosmology
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_Scopus_20250125
dc.titleScalar Field Cosmology in f(R,T) Gravity with Λ
dc.typeArticle

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