Kantowski-Sachs Holographic Cosmological Model in Saez-Ballester Theory of Gravitation

Abstract

In this paper, we consider the spatially homogeneous Kantowski-Sachs cosmological model filled with two minimally interacting fields, matter and holographic dark energy components in the frame work of scalar tensor theory proposed by Saez and Ballester (1986). To obtain a determinate solution of the field equations we have used the scalar expansion is proportional to the shear scalar. Some physical and geometrical properties of the model are also discussed.