Testing the viability of the interacting holographic dark energy model by using combined observational constraints
By C. Feng, Bin Wang, Y. Gong, R. Su. 2007
178 citations recorded by the source corpus.
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 for explaining the observed acceleration of our universe.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/1b6ae5d3c0f188b7a1ecc6fe39defc3e2225abbd
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In Astronomy and Astrophysics
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Citations in the corpus
- Holographic dark energy (2016, methodology): “In [326], by using the Glod04 SNIa sample, the shift parameter of the CMB from the WMAP3, the BAO measurement from the SDSS, the H(z) measurement and the lookback time data, Feng et al.”