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

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

2007-06-27

arxiv.org/abs/0706.4033v2

JCAP 0709:005,2007

Astronomy and Astrophysics

Astrophysics

15 pages, 9 figures, accepted for publication in JCAP

Scientific paper

10.1088/1475-7516/2007/09/005

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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