Magnetic versus baryonic jets for gamma-ray bursts.
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Pre-published on:
December 12, 2017
Published on:
November 11, 2020
Abstract
I discuss observed and theoretical constraints on the magnetization of gamma-ray burst (GRB) jets. Then, I describe a model based on the striped wind, and I explain how this model can help in solving the photon production problem in photospheric emission models of GRBs.
DOI: https://doi.org/10.22323/1.312.0067
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.