GRB 221009A: An ordinary nearby GRB with extraordinary observational properties
QB460-466
High Energy Astrophysical Phenomena (astro-ph.HE)
0103 physical sciences
FOS: Physical sciences
Gamma-ray bursts
Astrophysics
Astrophysics - High Energy Astrophysical Phenomena
01 natural sciences
DOI:
10.48550/arxiv.2303.10804
Publication Date:
2023-01-01
AUTHORS (19)
ABSTRACT
The gamma-ray burst GRB 221009A, known as the ``brightest-of-all-time" (BOAT), is closest energetic detected so far, with an energy of $E_{γ,\rm iso} \sim 10^{55}$ ergs. This study aims to assess its compatibility and luminosity distributions. Our analysis indicates that energy/luminosity function GRBs consistent across various redshift intervals, inclusion 221009A does not significantly impact at low redshifts. Additionally, our evaluation best-fitting result entire sample suggests expected number greater than $10^{55}$ ergs a 0.2, emergence functions within $\sim 2σ$ Poisson fluctuation error, still adhering principles small statistics. Furthermore, we find other bursts, defined \gtrsim10^{54} {\rm ergs}$, exhibit no significant differences in terms distributions $T_{90}$, minimum timescale, Amati relation, $E_{\rm γ,iso}$-$E_{\rm X,iso}$ $L_{γ,\rm iso}-Γ_0$ iso}-E_{\rm p,i}-Γ_0$ host galaxy properties, compared normal long GRBs. (including 221009A) likely have similar progenitor systems undergo dissipation radiation processes. generation may be due more extreme central engine properties or, likely, rarer viewing configuration quasi-universal structured jet.
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