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@ARTICLE{Aloisio:399161,
      author       = {Aloisio, Roberto and Boncioli, Denise and Di Matteo,
                      Armando and Grillo, Aurelio F. and Petrera, Sergio and
                      Salamida, Francesco and developers, SimProp},
      title        = {{S}im{P}rop v2r4: {M}onte {C}arlo simulation code for
                      {UHECR} propagation},
      journal      = {Journal of cosmology and astroparticle physics},
      volume       = {1711},
      number       = {11},
      issn         = {1475-7516},
      address      = {London},
      publisher    = {IOP},
      reportid     = {PUBDB-2018-00466, arXiv:1705.03729},
      pages        = {009},
      year         = {2017},
      note         = {© IOP Publishing Ltd and Sissa Medialab},
      abstract     = {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.},
      keywords     = {cosmic radiation: UHE (INSPIRE) / numerical calculations:
                      Monte Carlo (INSPIRE) / radiation: secondary (INSPIRE) /
                      propagation (INSPIRE) / electron positron (INSPIRE) /
                      observatory (INSPIRE) / adiabatic (INSPIRE) / energy loss
                      (INSPIRE) / redshift (INSPIRE) / cosmic background radiation
                      (INSPIRE) / magnetic field (INSPIRE) / infrared (INSPIRE) /
                      cross section (INSPIRE) / photon: background (INSPIRE) /
                      cascade: electromagnetic (INSPIRE) / Compton scattering:
                      inverse (INSPIRE) / nucleus: stability (INSPIRE) /
                      interaction (INSPIRE) / semileptonic decay (INSPIRE) /
                      neutrino (INSPIRE) / gamma ray: flux (INSPIRE) / energy:
                      injection (INSPIRE) / Lorentz (INSPIRE) / injection:
                      spectrum (INSPIRE) / density (INSPIRE)},
      cin          = {$Z_THAT$},
      ddc          = {530},
      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)29 / PUB:(DE-HGF)16},
      eprint       = {1705.03729},
      howpublished = {arXiv:1705.03729},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1705.03729;\%\%$},
      UT           = {WOS:000415003600001},
      doi          = {10.1088/1475-7516/2017/11/009},
      url          = {https://bib-pubdb1.desy.de/record/399161},
}