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arXiv · 0706.4033

Testing the viability of the interacting holographic dark energy model by using combined observational constraints

Chang Feng·Bin Wang·Yungui Gong·Ru-Keng Su
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Abstract

Using the data coming from the new 182 Gold type Ia supernova samples, the shift parameter of the Cosmic Microwave Background given by the three-year Wilkinson Microwave Anisotropy Probe observations, and the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey, $H(z)$ and lookback time measurements, we have performed a statistical joint analysis of the interacting holographic dark energy model. Consistent parameter estimations show us that the interacting holographic dark energy model is a viable candidate to explain the observed acceleration of our universe.

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Chang Feng, Bin Wang, Yungui Gong, Ru-Keng Su. 2007-08-15. Testing the viability of the interacting holographic dark energy model by using combined observational constraints. https://doi.org/10.1088/1475-7516%2F2007%2F09%2F005

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