Bianchi Type-Vih Universe Filed With Interacting Cold Dark Matter And Holographic Dark Energy

In the present work, we have solved Einstein field equations in presence of Holographic dark energy and interacting Dark matter in space-time describe by spatially homogeneous and anisotropic Bianchi type-VIh. The solution of field equations are obtained under the condition of the expansion scalar (θ ) is proportional to shear scalar (σ ). In order to distinguish between our dark energy model with other existing dark energy models, the State finder diagnostic is applied to the model. The physical and kinematical properties of the models are also discussed