Inflationary Scenario in Bianchi Type II Space with Bulk Viscosity in General Relativity

Abstract

This study is about bulk viscous inflationary model with flat potential under framework of LRS Bianchi type II metric. To drive relativistic solution of the field equations we choose theproportionally condition between coefficient of shear and expansion scalar which leads to asuitable relation  between the metric functions where n is the constant other than one. Some dynamical features of the universe are also discussed.