Notes on interacting holographic dark energy model in a closed universe
H. Mohseni Sadjadi and N. Vadood
Arxiv ID: 0806.2767•Last updated: 3/12/2021
We consider interacting holographic dark energy model in Friedmann Robertson Walker space time with positive spatial curvature and investigate the behavior of curvature parameter and dark energy density in accelerated expanding epoch. We also derive some conditions needed to cross the phantom divide line in this model.
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