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@ARTICLE{Aloisio:389649,
author = {Aloisio, Roberto and Boncioli, Denise and di Matteo,
Armando and Grillo, Aurelio F. and Petrera, Sergio and
Salamida, Francesco},
title = {{S}im{P}rop v2r4: {M}onte {C}arlo simulation code for
{UHECR} propagation},
reportid = {PUBDB-2017-08916, arXiv:1705.03729},
note = {21 pages, 3 figures; prepared for submission to JCAP. arXiv
admin note: text overlap with arXiv:1602.01239},
abstract = {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.},
cin = {$Z_THAT$},
cid = {$I:(DE-H253)Z_THAT-20210408$},
pnm = {613 - Matter and Radiation from the Universe (POF3-613) /
NEUCOS - Neutrinos and the origin of the cosmic rays
(646623)},
pid = {G:(DE-HGF)POF3-613 / G:(EU-Grant)646623},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)25 / PUB:(DE-HGF)29},
eprint = {1705.03729},
howpublished = {arXiv:1705.03729},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1705.03729;\%\%$},
url = {https://bib-pubdb1.desy.de/record/389649},
}