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arxiv: 1808.07481 · v2 · pith:KHLSZTVEnew · submitted 2018-08-22 · 🌌 astro-ph.HE

On the common origin of cosmic rays across the ankle and diffuse neutrinos at the highest energies from low-luminosity Gamma-Ray Bursts

classification 🌌 astro-ph.HE
keywords ankleburstscascadediffuseenergiesfluxgamma-rayhighest
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We demonstrate that the UHECRs produced in the nuclear cascade in the jet of Low-Luminosity Gamma-Ray Bursts (LL-GRBs) can describe the UHECR spectrum and composition and, at the same time, the diffuse neutrino flux at the highest energies. The radiation density in the source simultaneously controls the neutrino production and the development of the nuclear cascade, leading to a flux of nucleons and light nuclei describing even the cosmic-ray ankle at $5 \times 10^{18}$ eV. The derived source parameters are consistent with population studies, indicating a baryonic loading factor of about ten. Our results motivate the continued experimental search of LL-GRBs as a unique GRB population.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Ultraheavy Ultrahigh-Energy Cosmic Rays

    astro-ph.HE 2024-05 unverdicted novelty 7.0

    Ultraheavy nuclei have longer energy loss lengths at ≲300 EeV than lighter nuclei, allowing them to explain UHECRs above 100 EeV from sources like collapsars and neutron star mergers while predicting distinct shower maxima.

  2. Single-source-class interpretation of the diffuse astrophysical neutrino flux

    astro-ph.HE 2026-03 unverdicted novelty 4.0

    The diffuse astrophysical neutrino flux is interpreted as dominated by a single source class with dominant pγ production for target photon temperatures of 0.1-1 keV.