Bianchi type–I Model with Time Varying Λ and G: The Generalized Solution

Abstract

In this paper, we have investigated the homogeneous and anisotropic Bianchi type–I cosmological model with a time-varying Newtonian and cosmological constant. We have analytically solved Einstein’s field equations (EFEs) in the presence of a stiff-perfect fluid. We show that the analytical solution for the average scale factor for the generalized Friedman equation involves the hyper-geometric function. We have studied the physical and kinematical quantities of the model, and it is found that the universe becomes isotropic at late times.

Keywords

• bianchi metric
• anisotropic
• varying λ
• varying g “newtonian constant”