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@ARTICLE{deSousaFerreiraRodrigues:448235,
      author       = {de Sousa Ferreira Rodrigues, Xavier and Heinze, Jonas and
                      Palladino, Andrea and van Vliet, Arjen and Winter, Walter},
      title        = {{AGN} jets as the origin of {UHECR}s and perspectives for
                      the detection of {E}e{V} astrophysical neutrinos},
      reportid     = {PUBDB-2020-03344, arXiv:2003.08392. DESY-20-095},
      year         = {2021},
      note         = {[v1] Wed, 18 Mar 2020 : Blazar origin of the UHECRsand
                      perspectives for the detection of astrophysical source
                      neutrinos at EeV energies},
      abstract     = {We demonstrate that a population of Active Galactic Nuclei
                      (AGN) can describe the observed spectrum of
                      ultra-high-energy cosmic rays (UHECRs) at and above the
                      ankle, and that the dominant contribution comes from
                      low-luminosity BL Lacs. Such an AGN-only scenario is in
                      tension with UHECR composition observations above 10 EeV.
                      However, a sub-dominant contribution from high-luminosity
                      AGN reduces this tension and leads simultaneously to a
                      substantial neutrino flux that peaks at EeV energies. The
                      same emission also extends down to PeV energies, and is
                      therefore constrained by current IceCube limits. We also
                      show that the flux of neutrinos emitted from within the
                      sources should outshine the cosmogenic neutrinos produced
                      during the propagation of UHECRs. This result has profound
                      implications for ultra-high-energy ($\sim$EeV) neutrino
                      experiments, since additional search strategies can be used
                      for source neutrinos compared to cosmogenic neutrinos, such
                      as stacking searches, flare analyses, and multi-messenger
                      follow-ups.},
      keywords     = {cosmic radiation: UHE (INSPIRE) / cosmic radiation:
                      spectrum (INSPIRE) / neutrino: flux (INSPIRE) / neutrino:
                      energy: high (INSPIRE) / blazar (INSPIRE) / messenger
                      (INSPIRE) / propagation (INSPIRE) / stacking (INSPIRE)},
      cin          = {$Z_THAT$},
      cid          = {$I:(DE-H253)Z_THAT-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613) /
                      NEUCOS - Neutrinos and the origin of the cosmic rays
                      (646623)},
      pid          = {G:(DE-HGF)POF4-613 / G:(EU-Grant)646623},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2003.08392},
      howpublished = {arXiv:2003.08392},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2003.08392;\%\%$},
      doi          = {10.3204/PUBDB-2020-03344},
      url          = {https://bib-pubdb1.desy.de/record/448235},
}