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arXiv · 2307.16467

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

Hanbei Xie·Xiaodong Nong·Huifeng Wang·Bin Zhang·Zihao Li·Nan Liang
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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 are 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.

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Hanbei Xie, Xiaodong Nong, Huifeng Wang, Bin Zhang, Zihao Li, Nan Liang. 2023-07-31. Constraints on Cosmological Models with Gamma-Ray Bursts in Cosmology-Independent Way. https://doi.org/10.1142/s0218271824500731

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