Cosmological models with EoS parameters in f(T) theory of gravity

Abstract

We have presented cosmological models with equation of state (EoS) parameters in $$f(T)$$ theory of gravity, which is an extension of the teleparallel theory of gravity, where T is the torsion scalar. In this paper, we have used the EoS $$p{}_{\text{m}} = \omega \,\rho {}_{\text{m}}$$ and continuity equation. The cosmological evolution, different cases of fluids and their combination in $$f\left( T \right)$$ model are discussed. The physical and geometrical aspects of the models are also investigated.