The Holographic dark energy reexamined

Details The Holographic dark energy reexamined The Holographic dark energy reexamined

2004-12-19

arxiv.org/abs/hep-th/0412218v3

Phys.Rev. D72 (2005) 043510

Physics

High Energy Physics

High Energy Physics - Theory

divided into sections, add one figure, some typos corrected, references added, Accepted for publication in PRD; v3: some typos

Scientific paper

10.1103/PhysRevD.72.043510

We have reexamined the holographic dark energy model by considering the spatial curvature. We have refined the model parameter and observed that the holographic dark energy model does not behave as phantom model. Comparing the holographic dark energy model to the supernova observation alone, we found that the closed universe is favored. Combining with the Wilkinson Microwave Anisotropy Probe (WMAP) data, we obtained the reasonable value of the spatial curvature of our universe.

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