Magnetized dark energy cosmological models with time dependent cosmological term in Lyra geometry

In the present paper we have investigated a magnetized dark energy Bianchi type VI0 space time with time dependent cosmological term within the framework of Lyra's manifold with uniform and time varying displacement field. In order to obtain a determinate solution of the field equations we have assumed a new special law for the deceleration parameter proposed by Akarsu and Dereli and very recently used by Abdussattar and Prajapati. Without loss of generality, by taking into consideration the constant of integration to zero one particular model with some physical parameters are discussed more in detail. We have examined the isotropy and expansion of the universe