On the ultra-high energy cosmic ray horizon
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🌌 astro-ph
keywords
cosmicenergyhorizonsourcesultra-highabovecertaincompute
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We compute the ultra-high energy cosmic ray horizon, i.e. the distance up to which cosmic ray sources may significantly contribute to the fluxes above a certain threshold on the observed energies. We obtain results both for proton and heavy nuclei sources.
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