Bianchi type III inflationary universe with flat potential and stiff fluid distribution in general relativity

Abstract

In this study, we looked at the “Bianchi Type III stiff fluid cosmological model in general relativity”. To get an inflationary solution we have used appropriate condition between matric potential. Here n is non-negative integer and B and C are dependent function of time “t”. The structure characteristics of model are also pointed. The behaviour of the model under different physical conditions is also discussed.