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

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 Jing’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.