Abstract
We have examined spatially homogeneous and anisotropic cosmological models in the presence of two forms of dark energy (DE). We have calculated the exact solutions of the Einsteins field equations by assuming a special law of variation of Hubbles parameter [3] . Some physical parameters of the model are determined. From the point of kinematical behaviour we have also extended our work by deriving the analytic expressions for the look back time.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have