Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/51139
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Type: Journal article
Title: Interactions of UHE cosmic ray nuclei with radiation during acceleration: consequences for the spectrum and composition
Author: Allard, D.
Protheroe, R.
Citation: Astronomy and Astrophysics: a European journal, 2009; 502(3):803-815
Publisher: E D P Sciences
Issue Date: 2009
ISSN: 0004-6361
1432-0746
Statement of
Responsibility: 
D. Allard and R. J. Protheroe
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
Keywords: acceleration of particles -- nuclear reactions -- nucleosynthesis
abundances
Description: © ESO 2009
DOI: 10.1051/0004-6361/200911839
Grant ID: http://purl.org/au-research/grants/arc/DP0881006
Published version: http://dx.doi.org/10.1051/0004-6361/200911839
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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