Origin of the ankle in the ultrahigh energy cosmic ray spectrum, and of the extragalactic protons below it
Abstract
The sharp change in slope of the ultrahigh energy cosmic ray (UHECR) spectrum around 1 018.6 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 1 017.5 eV . Predictions for the spectrum and flavors of neutrinos resulting from this process are also presented.
- Publication:
-
Physical Review D
- Pub Date:
- December 2015
- DOI:
- 10.1103/PhysRevD.92.123001
- arXiv:
- arXiv:1505.02153
- Bibcode:
- 2015PhRvD..92l3001U
- Keywords:
-
- 98.70.Sa;
- 95.85.Ry;
- 96.50.sb;
- Cosmic rays;
- Neutrino muon pion and other elementary particles;
- cosmic rays;
- Composition energy spectra and interactions;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- extended discussion of source parameters, accepted for publication in PRD