Hadronic supercriticality as a trigger for GRB emission
Maria Petropoulou, Stavros Dimitrakoudis, Apostolos Mastichiadis,, Dimitrios Giannios

TL;DR
This paper investigates a hadronic model for gamma-ray burst emission, showing that supercritical energy transfer from protons to photons and neutrinos can produce observed spectra with high efficiency, under certain conditions.
Contribution
It introduces a minimal-parameter hadronic model demonstrating supercriticality as a trigger for GRB emission, supported by analytical and numerical analysis.
Findings
Supercriticality occurs when proton injection compactness exceeds a critical value.
Photon spectra become Band-like due to Comptonization in supercritical conditions.
Energy transfer efficiency to gamma-rays and neutrinos reaches approximately 30%.
Abstract
We explore a one-zone hadronic model that may be able to reproduce -ray burst (GRB) prompt emission with a minimum of free parameters. Assuming only that GRBs are efficient high-energy proton accelerators and without the presence of an ab initio photon field, we investigate the conditions under which the system becomes supercritical, i.e. there is a fast, non-linear transfer of energy from protons to secondary particles initiated by the spontaneous quenching of proton-produced -rays. We first show analytically that the transition to supercriticality occurs whenever the proton injection compactness exceeds a critical value, which favours high proton injection luminosities and a wide range of bulk Lorentz factors. The properties of supercriticality are then studied with a time-dependent numerical code that solves concurrently the coupled equations of proton, photon,…
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