# Constraints on Cosmological Models with Gamma-Ray Bursts in Cosmology-Independent Way

**Authors:** Hanbei Xie, Xiaodong Nong, Bin Zhang, Huifeng Wang, Zihao Li, Nan Liang  
**arXiv:** [2307.16467](https://arxiv.org/abs/2307.16467)  
**Date:** 2023-07-31  
**Summary page:** https://www.summarizepaper.com/fr/arxiv-id/2307.16467v1/

## Abstract

In this paper, we present a cosmology-independent method to constrain cosmological models from the latest 221 gamma-ray bursts (GRBs) sample, including 49 GRBs from Fermi catalog with the Amati relation (the $E_{\rm p}$-${E}_{\rm iso}$ correlation), which calibrated by using a Gaussian process from the Pantheon+ type Ia supernovae (SNe Ia) sample. With 182 GRBs at $0.8\le z\le8.2$ in the Hubble diagram and the latest observational Hubble data (OHD) by the Markov Chain Monte Carlo (MCMC) method, we obtained $\Omega_{\rm m}$ = $0.348^{+0.048}_{-0.066}$ and $h$ = $0.680^{+0.029}_{-0.029}$ for the flat $\Lambda$CDM model, and $\Omega_{\rm m}$ = $0.318^{+0.067}_{-0.059}$, $h$ = $0.704^{+0.055}_{-0.068}$, $w$ = $-1.21^{+0.32}_{-0.67}$ for the flat $w$CDM model. These results are consistent with those in which the coefficients of the Amati relation and the cosmological parameters fitted simultaneously.