Constraints on the interacting holographic dark energy model

Abstract

We examined the interacting holographic dark energy model in a universe with spatial curvature. Using the near-flatness condition and requiring that the universe is experiencing an accelerated expansion, we have constrained the parameter space of the model and found that the model can accommodate a transition of the dark energy from ${\omega }_D>-1$ to ${\omega }_D<-1$.

9 pages, 6 figures

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