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arXiv · 2209.10832

The Origin of the Photospheric Emission of GRB 220426A

Xin-Ying Song·Shuang-Nan Zhang·Ming-Yu Ge·Shu Zhang
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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 $η$ 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 $η$ with lower luminosity $L$ in the first few seconds, so that the trend of time-resolved $η-L$ can not be described as a monotonically positive correlation between $η$ and $L$. A hybrid outflow with almost completely thermalized Poynting flux could account for the quasi-thermal spectrum as well as large $η$. 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 $η-L$. 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.

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Xin-Ying Song, Shuang-Nan Zhang, Ming-Yu Ge, Shu Zhang. 2022-10-24. The Origin of the Photospheric Emission of GRB 220426A. https://doi.org/10.1093/mnras%2Fstac2764

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