Bianchi type \({VI}_{0}\) cosmological model for expanding universe with flat potential in general relativity

The focus of our study is on the Bianchi-type \({VI}_{0}\) ${\mathit{VI}}_0$ inflationary universe and how it behaves when a massless scalar field with a flat potential is present. Our goal is to identify an inflationary solution, which we achieved by identifying a flat region where the potential V remains constant. We have thoroughly examined the inflationary scenario of this model.