Modified Holographic Ricci Dark Energy Cosmological Model in Modified Theory of Gravity

Abstract

This work analyses a collection of solutions representing the modified holographic Ricci dark energy (MHRDE) cosmological model in modified f(R, T) gravity within the framework of the universe’s late-time accelerating expansion in an anisotropic axially symmetric cosmological model with pressureless matter substance. To solve the field equations, Chen and **g’s modified holographic Ricci dark energy, the hybrid expansion law, and a relationship between metric potentials are all used. The EoS, matter-energy density, anisotropic dark energy density, and deceleration cosmological parameters have been calculated. We looked at a few important features of the derived model to see if they were consistent with the recent findings.