Cosmological constraints on the generalized holographic dark energy

Details Cosmological constraints on the generalized holographic dark energy Cosmological constraints on the generalized holographic dark energy

2012-03-22

arxiv.org/abs/1203.4907v1

Eur. Phys. J. C (2011) 71: 1800

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

14 pages, 5 figures. arXiv admin note: significant text overlap with arXiv:1105.1868

Scientific paper

We use the Markov ChainMonte Carlo method to investigate global constraints on the generalized holographic (GH) dark energy with flat and non-flat universe from the current observed data: the Union2 dataset of type supernovae Ia (SNIa), high-redshift Gamma-Ray Bursts (GRBs), the observational Hubble data (OHD), the cluster X-ray gas mass fraction, the baryon acoustic oscillation (BAO), and the cosmic microwave background (CMB) data. The most stringent constraints on the GH model parameter are obtained. In addition, it is found that the equation of state for this generalized holographic dark energy can cross over the phantom boundary wde =-1.

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