Inhomogeneous generalization of Bianchi type VI_h String Cosmological Model for stiff perfect fluid distribution

We have investigated inhomogeneous generalization of Bianchi type VI_h string cosmological model for stiff perfect fluid distribution. To obtain the deterministic solution of Einstein's field equations, we assume that the isotropic pressure p is equal to string rest density ρ. Each of the cases 1 + h = 0 and 1 + h ≠ 0 gives rise to families of universe. The model obtained is expanding, shearing and non-rotating universe. Some physical and geometrical features of the model are also discussed.