Non-static plane-symmetric barrow holographic dark energy model in   gravity

Abstract

We construct Barrow holographic dark energy in the non-static, plane-symmetric universe. BHDE is based on the Barrow relation for horizon entropy (considering the Hubble horizon as the IR cut-off). We deal with the issue of locating solutions to the theory of gravity for non-static plane-symmetric cosmological models. Where the nonmetricity is responsible for the gravitational interaction. We obtain the equation of state parameter (EoS), the deceleration parameter, for the BHDE model to determine the cosmological evolution of the model.