Holographic Dark Energy in Bianchi Type VIo Space Time With Cosmological Constant A

In this manuscript we have studied minimally interacting field Dark matter and Holographic Dark energy in Bianchi type VIo cosmological model with cosmological constant A. The solution of Einstein’s field equations have been obtained by using relation between metric potential and shear velocity is proportional to scalar expansion and the special law of variation for Hubble parameter which gives a constant value of deceleration parameter. Some physical and geometrical aspects of the model are also discussed.