On the 'Loose' Constraint from IceCube Neutrino Non-Detection of GRB 230307A
arXiv:2307.16547 · doi:10.3847/1538-4357/ad02ef
Abstract
The recent extremely bright gamma-ray burst (GRB), GRB 230307A from a binary neutron star merger may offer a good probe for the production of GRB-neutrinos. Within the constraint from IceCube neutrino non-detection, the limits for key physical parameters of this burst are extracted in different scenarios including the fireball, Poynting-flux-dominated (PFD) and hybrid jet. Different from the former nearby `monsters' and due to its smaller isotropic equivalent radiated energy ( erg), the constraint seems loose if non-thermal neutrinos produced from photomeson interactions are the only consideration. However, a quasi-thermal neutrino emission from hadronuclear processes is constrained in this neutron-rich post-merger environment, and the upper limit of the allowed nucleon loading factor is about a few. Based on this, a discussion is presented on the possible prompt emission mechanism and jet composition for GRB 230307A in the context of multi-messenger astrophysics. It is worth noting that till now no GRB-neutrinos have been ever detected, even for the two brightest nearby GRBs ever observed (GRB 221009A and GRB 230307A) which have different dissipation mechanisms.
arXiv commentPublished in ApJ 958,133;accepted for publication in ApJ on Oct. 11; 13 pages, 3 figures. submitted on 2023.08.11. Minor revision according to the reviwer's suggestions on Oct. 02
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