Open AccessThe Hubble diagram extended to z ≫ 1: the gamma‐ray properties of gamma‐ray bursts confirm the Λ cold dark matter model
Author(s) -
Firmani C.,
AvilaReese V.,
Ghisellini G.,
Ghirlanda G.
Publication year - 2006
Publication title -
monthly notices of the royal astronomical society: letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.067
H-Index - 122
eISSN - 1745-3933
pISSN - 1745-3925
DOI - 10.1111/j.1745-3933.2006.00219.x
Subject(s) - physics , cosmic distance ladder , supernova , astrophysics , dark energy , gamma ray burst , redshift , equation of state , galaxy , cosmology , quantum mechanics
Tight constraints on cosmological parameters can be obtained with standard candles spanning a range of redshifts as large as possible. We propose to treat Type Ia supernovae (SNIa) and long gamma‐ray bursts (GRBs) as a single class of candles. Taking advantage of the recent release of the Supernova Legacy Survey and the recent finding of a tight correlation among the energetics and other prompt gamma‐ray emission properties of GRBs, we are able to standardize the luminosities/energetics of both classes of objects. In this way we can jointly use GRBs and SNIa as cosmological probes to constrain Ω m and Ω Λ and the parameters of the dark energy equation of state through the same Bayesian method that we have, so far, applied to GRBs alone. Despite the large disparity in number (115 SNIa versus 19 GRBs) we show that the constraints on Ω m and Ω Λ are greatly improved by the inclusion of GRBs. More importantly, the result of the combined sample is in excellent agreement with the ΛCDM concordance cosmological model and does not require an evolving equation of state for the dark energy.