Extending the Hubble diagram by gamma ray bursts
arXiv:0910.1678 · doi:10.1051/0004-6361/200912769
Abstract
A new method to constrain the cosmological equation of state is proposed by using combined samples of gamma-ray bursts (GRBs) and supernovae (SNeIa). The Chevallier-Polarski-Linder parameterization is adopted for the equation of state in order to find out a realistic approach to achieve the deceleration/acceleration transition phase of dark energy models. We find that GRBs, calibrated by SNeIa, could be good distance indicators capable of discriminating between cosmological models and CDM model at high redshift.
5 pages, 5 figures, to appear in Astron. & Astroph
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