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Propagation of UHECRs in cosmological backgrounds: some results from SimProp

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arxiv 1307.3895 v1 pith:7QN2XIQW submitted 2013-07-15 astro-ph.HE astro-ph.CO

R. Aloisio , D. Boncioli , A. Di Matteo , A.F. Grillo , S. Petrera , F. Salamida This is my paper
classification astro-ph.HEastro-ph.CO
keywords nucleiuhecrapproachbackgroundscodecosmologicalpropagationresults
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Ultra-High-Energy Cosmic Ray (UHECR) nuclei propagating in cosmological radiation backgrounds produce secondary particles detectable at Earth. SimProp is a one dimensional code for extragalactic propagation of UHECR nuclei, inspired by the kinetic approach of Aloisio et al. As in this approach, only a subset of nuclei and nuclear channels are used as representative. We discuss the validation of the code and present applications to UHECR experimental results. In particular we present the expected fluxes of neutrinos produced in some astrophysical scenario.

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