Testing Dark Energy Models with Gamma-Ray Bursts Calibrated from the Observational Data through a Gaussian Process
arXiv:2212.14291 · doi:10.1093/mnras/stad838
Abstract
We use a cosmology-independent method to calibrate gamma-ray burst (GRB) from the observational Hubble data (OHD) with the cosmic chronometers method. By using Gaussian Process to reconstruct OHD, we calibrate the Amati relation (--) to construct a GRB Hubble diagram with the A118 data set, and constrain Dark Energy models in a flat space with the Markov Chain Monte Carlo numerical method. With the cosmology-independent GRBs at in the A118 data set and the Pantheon sample of type Ia supernovae (SNe Ia) at , we obtained = , = , = , = for the flat Chevallier-Polarski-Linder model at the 1 confidence level. We find no significant evidence supporting deviations from the standard CDM model.
arXiv comment8 pages, 8 figures, 3 tables, accepted for publication in MNRAS, now matches the editorially revised version
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