In this paper we present non-singular Bianchi types I and V cosmological models, in the presence of bulk viscous fluid and within the framework of f(R,T) gravity theory. Exact solutions to the field equations are obtained by choosing a particular form of the function f(R,T) and a special value for the average scale factor of the model, which corresponds to a time- dependent deceleration parameter. The cosmological models initially accelerate for a certain period of time and thereafter decelerate. The physical and kinematical properties of the models of the universe are discussed. © 2014 Versita Warsaw and Springer-Verlag Wien.
CITATION STYLE
Ram, S., & Kumari, P. (2014). Bianchi types I and V bulk viscous fluid cosmological models in f(R, T) gravity theory. Central European Journal of Physics, 12(10), 744–754. https://doi.org/10.2478/s11534-014-0494-3
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