摘要

Anisotropic dark energy model is constructed by constraining the Hubble parameter at the back drop of Bianchi-I space-time in the frame work of General Relativity. It is observed that due to anisotropy, the energy density is negative initially and it became positive in the absence of anisotropy. From a state finder diagnosis, it is found that our model is having similar behaviour like ACDM model.

  • 出版日期2015-12