Bianchi Type-III Cosmological Models with Time Dependent Displacement Vector for Barotropic Fluid Distribution in Lyra Geometry

Bianchi Type-III cosmological models for perfect fluid distribution with time dependent displacement field in the framework of Lyra geometry are investigated. To get the deterministic model of the universe, we have assumed two conditions (i) shear (sigma) is proportional to the expansion (theta). This leads to B = C(n) where B and C are metric potentials and n is a constant. (ii) Universe is filled with barotropic fluid distribution which leads to p = gamma rho, 0 <= gamma <= 1, p being isotropic pressure and rho the energy density. The physical and geometrical aspects of the model with a special case and singularities in the models are also discussed.