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The Holographic dark energy revisited

Yun-gui Gong
(
- CUPT, Chongqing
)
,
Bin Wang
(
- Fudan U.
)
,
Yuan-Zhong Zhang
(
- CCAST World Lab, Beijing and
- Beijing, Inst. Theor. Phys.
)

Dec, 2004

5 pages

Published in:

Phys.Rev.D 72 (2005) 043510

e-Print:

hep-th/0412218 [hep-th]

DOI:

10.1103/PhysRevD.72.043510

View in:

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Abstract:

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.

98.80.Cq
98.80.Es
dark energy
holography
supernova
cosmic background radiation
numerical calculations: interpretation of experiments

References(78)

Figures(0)

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