UHE nuclei propagation and the interpretation of the ankle in the cosmic-ray spectrum

Details UHE nuclei propagation and the interpretation of the ankle in the cosmic-ray spectrum UHE nuclei propagation and the interpretation of the ankle in the cosmic-ray spectrum

2005-05-27

arxiv.org/abs/astro-ph/0505566v2

Astron.Astrophys.443:L29-L32,2005

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, submitted to A&A Letters (minor changes, two figures replaced, two references added)

Scientific paper

10.1051/0004-6361:200500199

We consider the stochastic propagation of high-energy protons and nuclei in the cosmological microwave and infrared backgrounds, using revised photonuclear cross-sections and following primary and secondary nuclei in the full 2D nuclear chart. We confirm earlier results showing that the high-energy data can be fit with a pure proton extragalactic cosmic ray (EGCR) component if the source spectrum is \propto E^{-2.6}. In this case the ankle in the CR spectrum may be interpreted as a pair-production dip associated with the propagation. We show that when heavier nuclei are included in the source with a composition similar to that of Galactic cosmic-rays (GCRs), the pair-production dip is not present unless the proton fraction is higher than 85%. In the mixed composition case, the ankle recovers the past interpretation as the transition from GCRs to EGCRs and the highest energy data can be explained by a harder source spectrum \propto E^{-2.2} - E^{-2.3}, reminiscent of relativistic shock acceleration predictions, and in good agreement with the GCR data at low-energy and holistic scenarios.

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