Aygün, SezginAktaş, CanSahoo, Pradyumn KumarBishi, Binaya K.2025-01-272025-01-2720180202-2893https://doi.org/10.1134/S0202289318030039https://hdl.handle.net/20.500.12428/12858We 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.eninfo:eu-repo/semantics/closedAccessArticle24330230710.1134/S0202289318030039Q4WOS:0004426273000122-s2.0-85052249042Q3