Volumetric expansions of accelerating unstable cosmological models with a quadratic form of equation of state
In this paper, we derive the field equations towards f (R) gravity (where is the Ricci scalar) with the help of a locally rotationally symmetric spatially homogeneous and anisotropic Bianchi type-I space-time, in the presence of perfect fluid with Quadratic form of Equation of State. Here we obtained the solutions of the field equations using volumetric power and exponential law of expansion, under some specific plausible physical conditions. The stability factor of the model is initially positive which satisfy that the velocity of sound should be less than the velocity of light i.e.