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In this paper we have obtained axially symmetric Bianchi type-I cosmological models for perfect fluid distribution in the context of Lyra’s manifold. Exact solutions of the field equations are obtained by assuming the expansion  in the model is proportional to the shear . This leads to the condition n B A  where A and B are scale factors and ) 0 ( n is a constant. Some kinematical and physical parameters of the model have been discussed. The solutions are compatible with recent observations.

Exact Solutions of Axially Symmetric Bianchi Type-I Cosmological Model in Lyra Geometry