Two-component jet model for the afterglow emission of GRB 201216C and GRB 221009A and implications for jet structure of very-high-energy gamma-ray bursts

TL;DR

This paper demonstrates that a two-component jet model with narrow and wide jets can explain the VHE afterglow emissions of GRBs 201216C and 221009A, providing insights into their jet structures and energies.

Contribution

The study extends the two-component jet model to additional VHE GRBs, showing its effectiveness in explaining their afterglow spectra and light curves.

Findings

VHE spectra and light curves fit the two-component jet model

Typical collimation-corrected energies are 5×10^{49} erg and 5×10^{50} erg

Narrow jet of GRB 221009A has an unusually small opening angle

Abstract

In recent years, afterglow emission in the very-high-energy (VHE) band above 100 GeV has been clearly detected for at least five gamma-ray bursts (GRBs 180720B, 190114C, 190829A, 201216C and 221009A). For some of these VHE GRBs, we previously proposed a two-component jet model, consisting of two uniform jets with narrow and wide opening angles to explain their multiwavelength afterglows including VHE gamma rays. In this paper, we show that the VHE spectra and light curves of GRBs 201216C and 221009A can also be reasonably explained by our two-component jet model, based on two top-hat jets propagating into a constant-density circumburst medium. We find that for the five VHE GRBs, the collimation-corrected kinetic energies of the narrow and wide jets have typical values of 5*10^{49} erg and 5*10^{50} erg, respectively. We discuss the similarities and differences among the VHE GRBs, and the implications for the structure of their jets. In agreement with previous studies, the narrow jet of GRB 221009A has an atypically small opening angle, so that its intrinsic, collimation-corrected energy remains within a plausible range despite the unusually large isotropic-equivalent energy.