Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-12-03
Phys.Lett.B658:95-100,2008
Astronomy and Astrophysics
Astrophysics
7 pages and 3 figures. Replaced with version accepted for publication in Phys. Lett. B
Scientific paper
10.1016/j.physletb.2007.10.053
In this paper we analyze the constraints on the property of dark energy from cosmological observations. Together with SNe Ia Gold sample, WMAP, SDSS and 2dFGRS data, we include 69 long Gamma-Ray Bursts (GRBs) data in our study and perform global fitting using Markov Chain Monte Carlo (MCMC) technique. Dark energy perturbations are explicitly considered. We pay particular attention to the time evolution of the equation of state of dark energy parameterized as $w_{DE}=w_0+w_a(1-a)$ with $a$ the scale factor of the universe, emphasizing the complementarity of high redshift GRBs to other cosmological probes. It is found that the constraints on dark energy become stringent by taking into account high redshift GRBs, especially for $w_a$, which delineates the evolution of dark energy.
Dai Zigao
Fan Zuhui
Li Hong
Su Meng
Zhang Xinmin
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