Interacting Holographic Dark Energy in Bianchi Type-V Universe with Variable Deceleration Parameter

Abstract

The present study deals with spatially homogeneous and anisotropic Bianchi Type-V universe filled with interacting dark matter and holographic dark energy. The exact solutions of Einstein's equations are obtained by using the variable deceleration parameter in the form ( ) ( ) ( ) 1 sinh n a t t α = (Chawla et al. [1]). The physical properties of the model are obtained and discussed in details.