Preprint PUBDB-2020-03344

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AGN jets as the origin of UHECRs and perspectives for the detection of EeV astrophysical neutrinos

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2021

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Report No.: DESY-20-095; arXiv:2003.08392

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.

Keyword(s): cosmic radiation: UHE ; cosmic radiation: spectrum ; neutrino: flux ; neutrino: energy: high ; blazar ; messenger ; propagation ; stacking


Note: [v1] Wed, 18 Mar 2020 : Blazar origin of the UHECRsand perspectives for the detection of astrophysical source neutrinos at EeV energies

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
  2. NEUCOS - Neutrinos and the origin of the cosmic rays (646623) (646623)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2020
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http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Journal Article  ;  ;  ;  ;
Active galactic nuclei jets as the origin of ultrahigh-energy cosmic rays and perspectives for the detection of astrophysical source neutrinos at EeV energies
Physical review letters 126(19), 191101 (1-6) () [10.1103/PhysRevLett.126.191101]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2020-09-10, last modified 2024-02-27


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