Interactions of UHE cosmic ray nuclei with radiation during acceleration: consequences for the spectrum and composition

Free access article

Issue		A&A Volume 502, Number 3, August II 2009


Page(s)		803 - 815
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361/200911839
Published online		15 June 2009

A&A 502, 803-815 (2009)
DOI: 10.1051/0004-6361/200911839

Interactions of UHE cosmic ray nuclei with radiation during acceleration: consequences for the spectrum and composition

D. Allard¹ and R. J. Protheroe²

¹ Laboratoire Astroparticule et Cosmologie (APC), Université Paris 7/CNRS, 10 rue A. Domon et L. Duquet, 75205 Paris Cedex 13, France
e-mail: denis.allard@apc.univ-paris7.fr
² Department of Physics, The University of Adelaide, SA 5005, Australia
e-mail: rprother@physics.adelaide.edu.au

Received 12 February 2009 / Accepted 28 May 2009

Abstract
In this paper, we study the diffusive shock acceleration of cosmic-ray protons and nuclei, taking all the relevant interaction processes with photon backgrounds into account. We investigate how the competition between protons and nuclei is modified by such acceleration parameters as the acceleration rate, its rigidity dependence, the photon density, and the confinement capability of the sources. We find that protons are likely to be accelerated to higher energies than nuclei in the case of interaction-limited acceleration processes, whereas nuclei are accelerated to higher energies than protons for confinement-limited acceleration. Finally, we discuss our results in the context of possible astrophysical accelerators and in the light of recent cosmic-ray data.

Key words: acceleration of particles -- nuclear reactions -- nucleosynthesis, abundances

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