LAUSR

We have presented cosmological models with equation of state (EoS) parameters in $$f(T)$$ 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 $$p{}_{\text{m}} = \omega \,\rho {}_{\text{m}}$$ p m = ω ρ m and continuity equation. The cosmological evolution, different cases of fluids and their combination in $$f\left( T \right)$$ f T model are discussed. The physical and geometrical aspects of the models are also investigated.