Abstract:
We discussed Bianchi type-I bulk viscous cosmological model of inflationary universe in GR. To get deterministic model of the universe, it has been considered a flat region in which potential v (Φ) = constant where Φ is Higg’s field and also considered coefficient of bulk (ζ) is inversely proportional to the expansion
θ .The physical and geometrical aspects of the model in the context of inflationary scenario are also discussed.