{ "id": "2209.10832", "version": "v1", "published": "2022-09-22T07:37:45.000Z", "updated": "2022-09-22T07:37:45.000Z", "title": "The Origin of the Photospheric Emission of GRB 220426A", "authors": [ "Xin-Ying Song", "Shuang-Nan Zhang", "Ming-Yu Ge", "Shu Zhang" ], "comment": "15 pages, 7 figures, accepted for publication in MNRAS on 2022 September 20", "categories": [ "astro-ph.HE" ], "abstract": "GRB 220426A is a bright gamma-ray burst (GRB) dominated by the photospheric emission. We perform several tests to speculate the origin of this photospheric emission. The dimensionless entropy $\\eta$ is large, which is not usual if we assume that it is a pure hot fireball launched by neutrino-antineutrino annihilation mechanism only. Moreover, the outflow has larger $\\eta$ with lower luminosity $L$ in the first few seconds, so that the trend of time-resolved $\\eta-L$ can not be described as a monotonically positive correlation between $\\eta$ and $L$. A hybrid outflow with almost completely thermalized Poynting flux could account for the quasi-thermal spectrum as well as large $\\eta$. More importantly, the existence of magnetic field could affect the proton density and neutron-proton coupling effect, so that it could account for the observed trend of time-resolved $\\eta-L$. The other origins for the photospheric emission, such as non-dissipative hybrid outflow or magnetic reconnection, are not supported because their radiation efficiencies are low, which is not consistent with non-detection of the afterglow for GRB 220426A. Therefore, we think the hybrid outflow may be the most likely origin.", "revisions": [ { "version": "v1", "updated": "2022-09-22T07:37:45.000Z" } ], "analyses": { "keywords": [ "photospheric emission", "grb 220426a", "hybrid outflow", "neutrino-antineutrino annihilation mechanism", "bright gamma-ray burst" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable" } } }