Proton Synchrotron Origin of the Very-high-energy Emission of GRB 190114C

Proton Synchrotron Origin of the Very-high-energy Emission of GRB 190114C

We consider here a proton-synchrotron model to explain the MAGIC observation of GRB 190114C afterglow in the energy band of 0.2–1 TeV, while the X-ray spectra are explained by electron-synchrotron emission. Given the uncertainty of the particle acceleration process, we consider several variations of...

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Bibliographic Details
Main Authors:	Hebzibha Isravel, Asaf Pe’er, Damien Bégué
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Series:	The Astrophysical Journal
Subjects:	Gamma-ray bursts Interstellar synchrotron emission
Online Access:	https://doi.org/10.3847/1538-4357/acec73

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