Interacting Two Fluid Dark Energy Bianchi Type-I Radiating Cosmological Model in f(R) Gravity

Abstract

In this paper, we have investigated some features of purely past decelerated to present accelerating locally rotationally symmetric Bianchi type-I cosmological model in the presence of interacting two fluids namely matter and dark energy in the framework of f(R) theory of gravity. In this study we have produced the solution of field equations towards hybrid expansion law which makes the model past decelerated to present accelerating expansion. It is observed that the stable Universe has point-type singularity with an equation of state parameter showing Quintessence region and evolving towards ΛCDM which may also be established for the current accelerated expansion of the Universe.