Constraints on the interacting holographic dark energy model

Details Constraints on the interacting holographic dark energy model Constraints on the interacting holographic dark energy model

2005-09-14

arxiv.org/abs/hep-th/0509107v2

Phys.Lett. B637 (2006) 357-361

Physics

High Energy Physics

High Energy Physics - Theory

9 pages, 6 figures

Scientific paper

10.1016/j.physletb.2006.04.009

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 $\omega_D<-1$.

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