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Cited by 564

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The Acceleration of Ultra--High-Energy Cosmic Rays in Gamma-Ray Bursts

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Vietri, Mario·1995·The Astrophysical Journal

Abstract

Ultra-high-energy cosmic rays (UHECRs) are roughly isotropic and attain very large energies, E ≳ 3 × 1020 eV. Conventional models fail to explain both facts. I show here that acceleration of UHECRs in gamma-ray bursts (GRBs) satisfies both observational constraints. Using the Mészáros & Rees model (see their recent work) of GRBs as due to hyperrelativistic shocks, I show that the highest energies that can be attained thusly are E ≌ 1020 θ-5/3/ n15/6 eV, explaining the energy of the Bird et al. event (described in their recent work) even without beaming. The traditional photopion catastrophe affecting UHECR acceleration in active galactic nuclei is circumvented. An order of magnitude estimate shows that the total energy flux of UHECRs at Earth is also correctly reproduced. A test of the model based upon the UHECRs' distribution upon the plane of the sky is briefly discussed.

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Metadata

Authors
Vietri, M.
Venue
The Astrophysical Journal
Published
1995-11
Volume
453
Pages
883
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1992960149
Cited by
564
References
0
FWCI
9.11
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Acceleration of Ultra--High-Energy Cosmic Rays in Gamma-Ray Bursts. https://app.cochat.ai/papers/10.1086/176448
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Vietri, M. (1995). The Acceleration of Ultra--High-Energy Cosmic Rays in Gamma-Ray Bursts. The Astrophysical Journal. https://doi.org/10.1086/176448

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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.