Cosmology with gamma-ray bursts
M. DemiańskiDepartment of Astronomy, Williams College, Williamstown, MA 01267, USAE. PiedipalumboDipartimento di Fisica, Università degli Studi di Napoli Federico II, Compl. Univ. Monte S. Angelo, 80126 Napoli, ItalyD. SawantDepartment of Physics, University of Nice Sophia Antipolis, Parc Valrose, 06034 Nice Cedex 2, FranceL. AmatiINAF–IASF, Sezione di Bologna, via Gobetti 101, 40129 Bologna, Italy
2016en
ABI
Аннотация
Context. Gamma-ray bursts (GRBs) are the most energetics explosions in the Universe. They are detectable up to very high redshifts. They may therefore be used to study the expansion rate of the Universe and to investigate the observational properties of dark energy, provided that empirical correlations between spectral and intensity properties are appropriately calibrated.
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