In this paper, we attempt to study spatially homogeneous Bianchi types-III, V, VI_0 \& VI_h cosmological models in f(R, T) theory of gravity. Here the models are obtained by assuming forms of the function f(R, T) as f(R, T)= R + 2f(T) and f(R, T) = f_1(R)+f_2(T). The exact solutions of Einstein's field equations (EFEs) have been obtained for two different types of physically viable cosmologies using a special form of Hubble parameter (HP). The physical and geometrical properties of these models have been discussed and expressions for the Ricci scalar R in each case are obtained.
Bianchi types-III V VI_0 \& VI_h f(R-T) theory of gravity Cosmic time Cosmological constant Exact solutions Hubble parameter Variational principle
Primary Language | English |
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Subjects | Mathematical Sciences |
Journal Section | Articles |
Authors | |
Publication Date | December 26, 2019 |
Submission Date | June 21, 2018 |
Acceptance Date | April 30, 2019 |
Published in Issue | Year 2019 |
Journal of Mathematical Sciences and Modelling
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