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· 2024 · arXiv 2403.02072

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astro-ph.HE 1

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2024 1

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Ultraheavy Ultrahigh-Energy Cosmic Rays

astro-ph.HE · 2024-05-27 · 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.

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  • Ultraheavy Ultrahigh-Energy Cosmic Rays astro-ph.HE · 2024-05-27 · unverdicted · none · ref 54

    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.