Cosmological models with Magnetized Anisotropic Dark Energy in Lyra Geometry

We have studiedanisotropic and homogenous Bianchi Type VI0 space-time under the assumption of anisotropy of the fluid within the frame work of Lyra manifold in the presence and absence of magnetism. A special form of deceleration parameter which gives an early deceleration and late time accelerating cosmological models has been utilized to solve the field equations. The physical and geometrical behaviors of the model are also discussed.