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SimProp v2r4: Monte Carlo simulation code for UHECR propagation

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arxiv 1705.03729 v4 pith:JR6FCBIW submitted 2017-05-10 astro-ph.HE astro-ph.IM

SimProp v2r4: Monte Carlo simulation code for UHECR propagation

Roberto Aloisio , Denise Boncioli , Armando di Matteo , Aurelio F. Grillo , Sergio Petrera , Francesco Salamida This is my paper
classification astro-ph.HE astro-ph.IM
keywords codecosmicenergypropagationrayssimpropultra-highcarlo
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We introduce the new version of SimProp, a Monte Carlo code for simulating the propagation of ultra-high energy cosmic rays in intergalactic space. This version, SimProp v2r4, together with an overall improvement of the code capabilities with a substantial reduction in the computation time, also computes secondary cosmogenic particles such as electron-positron pairs and gamma rays produced during the propagation of ultra-high energy cosmic rays. As recently pointed out by several authors, the flux of this secondary radiation and its products, within reach of the current observatories, provides useful information about models of ultra-high energy cosmic ray sources which would be hard to discriminate otherwise.

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Cited by 2 Pith papers

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    astro-ph.HE 2026-06 unverdicted novelty 4.0

    Sets upper limits on primordial black hole dark matter fraction using extragalactic gamma-ray background, claiming these are the tightest indirect constraints for the mass range.