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

TL;DR
This paper proposes a photo-disintegration mechanism near UHECR sources to explain the ankle feature and composition of extragalactic cosmic rays, matching observed spectra and neutrino predictions.
Contribution
It introduces a new model where photo-disintegration near sources accounts for the spectrum and composition of extragalactic cosmic rays below the ankle.
Findings
Reproduces the observed spectrum and composition above 10^17.5 eV.
Predicts neutrino fluxes consistent with observations.
Provides a unified explanation for the ankle and extragalactic protons.
Abstract
The sharp change in slope of the ultrahigh 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 and intermediate composition above, has proved exceedingly challenging to understand theoretically, without fine-tuning. We propose a mechanism whereby photo-disintegration of ultrahigh energy nuclei in the region surrounding a UHECR accelerator accounts for the observed spectrum and inferred composition at Earth. For suitable source conditions, the model reproduces the spectrum and the composition over the entire extragalactic cosmic ray energy range, i.e. above 10^17.5 eV. Predictions for the spectrum and flavors of neutrinos resulting from this process are also presented.
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