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001     389649
005     20240227162242.0
024 7 _ |a arXiv:1705.03729
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037 _ _ |a PUBDB-2017-08916
041 _ _ |a English
088 1 _ |a arXiv:1705.03729
088 _ _ |a arXiv:1705.03729
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100 1 _ |a Aloisio, Roberto
|b 0
245 _ _ |a SimProp v2r4: Monte Carlo simulation code for UHECR propagation
336 7 _ |a Preprint
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336 7 _ |a ARTICLE
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500 _ _ |a 21 pages, 3 figures; prepared for submission to JCAP. arXiv admin note: text overlap with arXiv:1602.01239
520 _ _ |a We introduce the new version of SimProp, a Monte Carlo code for simulating the propagation of ultra-high energy cosmic rays in the intergalactic space. This version, SimProp v2r4, together with an overall improvement of the code capabilities with a substantial reduction of 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.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
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536 _ _ |a NEUCOS - Neutrinos and the origin of the cosmic rays (646623)
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700 1 _ |a Boncioli, Denise
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700 1 _ |a di Matteo, Armando
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700 1 _ |a Grillo, Aurelio F.
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700 1 _ |a Petrera, Sergio
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700 1 _ |a Salamida, Francesco
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910 1 _ |a Deutsches Elektronen-Synchrotron
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913 1 _ |a DE-HGF
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914 1 _ |y 2017
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915 _ _ |a Published
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