Towards a new model-independent calibration of Gamma-Ray Bursts
arxiv(2024)
摘要
Current data on baryon acoustic oscillations and Supernovae of Type Ia cover
up to z∼2.5. These low-z observations play a very important role in the
determination of cosmological parameters and have been widely used to constrain
the ΛCDM and models beyond the standard. To extend this investigation
to higher redshifts, Gamma-Ray Bursts (GRBs) stand out as one of the most
promising observables since can probe the universe up to z∼9.4. The use of
GRB correlations is still a challenge due to the spread in their intrinsic
properties. In this work, we propose an innovative and cosmology-independent
method of calibration of the so-called 3D Dainotti correlation. We employ
state-of-the-art data on Cosmic Chronometers (CCH) at z≲2 and use the
Gaussian Processes Bayesian reconstruction tool. To match the CCH redshift
range, we select 20 long GRBs in 0.553 ≤ z ≤ 1.96 from the Platinum
sample, which consists of well-defined GRB plateau properties that obey the
fundamental plane relation. To ensure the generality of our method, we verify
that the choice of priors on the parameters of the Dainotti relation and the
modelling of CCH uncertainties and covariance have negligible impact on our
results. Moreover, we consider the case in which the redshift evolution of the
physical features of the plane is accounted for. We find that the use of CCH
allows us to identify a sub-sample of GRBs that adhere even more closely to the
fundamental plane relation, with an intrinsic scatter of
σ_int=0.20^+0.03_-0.05 obtained in this analysis when evolutionary
effects are considered. In an epoch in which we strive to reduce uncertainties
on the variables of the GRB correlations to tighten constraints on cosmological
parameters, we have found a novel model-independent approach to pinpoint a
sub-sample that can thus represent a valuable set of standardizable candles.
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