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Nuclear Composition of Gamma‐Ray Burst Fireballs

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Beloborodov, Andrei M.·2003·The Astrophysical Journal

Abstract

We study three processes that shape the nuclear composition of gamma-ray burst (GRB) fireballs: (1) neutronization in the central engine, (2) nucleosynthesis in the fireball as it expands and cools, and (3) spallation of nuclei in subsequent internal shocks. The fireballs are found to have a neutron excess and a marginally successful nucleosynthesis. They are composed of free nucleons, α-particles, and deuterium. A robust result is the survival of a significant neutron component, which has important implications. First, as shown in previous works, neutrons can lead to observable multi-GeV neutrino emission. Second, as we show in an accompanying paper, neutrons impact the explosion dynamics at radii up to 10 17 cm and change the mechanism of the GRB afterglow emission.

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Authors
Beloborodov, A. M.
Venue
The Astrophysical Journal
Published
2003-05-10
Volume
588
Issue
2
Pages
931-944
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2029784035
Cited by
196
References
0
FWCI
7.35
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Nuclear Composition of Gamma‐Ray Burst Fireballs. https://app.cochat.ai/papers/10.1086/374217
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Beloborodov, A. M. (2003). Nuclear Composition of Gamma‐Ray Burst Fireballs. The Astrophysical Journal. https://doi.org/10.1086/374217

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.