Bianchi Type I Tilted Cosmological Model for Barotropic Perfect Fluid Distribution with Heat Conduction in General Relativity

Bianchi Type I tilted cosmological model for barotropic perfect fluid distribution with heat conduction is investigated. To get the deterministic solution, we have assumed barotropic condition p = gamma is an element of,0 <= gamma <= I1, p being isotropic pressure, E the matter density and a supplementary condition between metric potentials A, B, C as A = (BC)n where n is the constant. To get the model in terms of cosmic time, we have also discussed some special cases. The physical aspects of the model are also discussed.