Anisotropic Bianchi type VI° cosmological Model in Self-Creation Theory of Gravitation

In this paper, Anisotropic Bianchi VI° cosmological model is investigated in the presence of perfect fluid coupled with electromagnetic field in Self–Creation Theory of Gravitation. The physical condition that is shear scalar is directly proportional to the expansion scalar is used to obtain the solution of the field equations. The physical and geometrical properties of the obtained model are discussed. Also, we study the thermodynamic quantities (Entropy, Enthalpy, Gibbs energy and Helmholtz energy) of the universe with help of the scalar field ∅ . In addition to this, we studied the Statefinder diagnostic pair and jerk parameter of the universe.