The Holographic dark energy reexamined

Bin Wang; Yuan-Zhong Zhang; Yungui Gong

The Holographic dark energy reexamined

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arxiv hep-th/0412218 v3 pith:D4IJALWX submitted 2004-12-19 hep-th astro-phgr-qc

Yungui Gong , Bin Wang , Yuan-Zhong Zhang This is my paper · ORCID

classification hep-thastro-phgr-qc

keywords modeldarkenergyholographiccurvaturereexaminedspatialuniverse

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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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