Origin of the ankle in the ultra-high energy cosmic ray spectrum and of the extragalactic protons below it
Glennys R. Farrar, Michael Unger, Luis A. Anchordoqui

TL;DR
This paper proposes that photo-disintegration of ultra-high energy nuclei near cosmic ray sources explains the spectral features and composition of extragalactic cosmic rays, with implications for neutrino signals.
Contribution
It introduces a model where photo-disintegration near sources accounts for the observed spectrum and composition of extragalactic UHECRs, explaining the ankle feature.
Findings
Photo-disintegration naturally reproduces the observed spectrum.
The model predicts specific neutrino signatures.
Explains the transition from light to intermediate composition.
Abstract
The sharp change in slope of the ultra-high energy cosmic ray (UHECR) spectrum around 10^{18.6} eV (the ankle), combined with evidence of a light but extragalactic component near and below the ankle which evolves to intermediate composition above, has proved exceedingly challenging to understand theoretically. We show that for a range of source conditions, photo-disintegration of ultra-high energy nuclei in the region surrounding a UHECR accelerator naturally accounts for the observed spectrum and composition of the entire extragalactic component, which dominates above about 10^{17.5} eV. The mechanism has a clear signature in the spectrum and flavors of neutrinos.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
