2005/04/27 by T. Di Girolamo, R. Catena, M. Vietri +1 · 1 citation
Physics and Astronomy · #astro-ph #gr-qc
paper · pdf · doi:10.1088/1475-7516/2005/04/008
published as JCAP.0504:008,2005 · 21 pages, 4 figures
arxiv created 2005/04/27 · arxiv updated 2009/12/01
Using the narrow clustering of the geometrically corrected gamma-ray energies released by gamma-ray bursts, we investigate the possibility of using these sources as standard candles to probe cosmological parameters such as the matter density Omegam and the cosmological constant energy density OmegaLambda. By simulating different samples of gamma-ray bursts, we find that Omegam can be determined with accuracy ~7% with data from 300 sources. We also show that, if Omega = 1 is due to a quintessence field, some of the models proposed in the literature may be discriminated from a Universe with cosmological constant, by a similar-sized sample of gamma-ray bursts.