Article Dans Une Revue JETP Lett. Année : 2021

Radio-to-Gamma-Ray Synchrotron and Neutrino Emission from Proton–Proton Interactions in Active Galactic Nuclei

Résumé

We explore possible physical origin of correlation between radio wave and very-high-energy neutrino emission in active galactic nuclei (AGN), suggested by recently reported evidence for correlation between neutrino arrival directions and positions of brightest radio-loud AGN. We show that such correlation is expected if both synchrotron emitting electrons and neutrinos originate from decays of charged pions produced in proton-proton interactions in parsec-scale relativistic jet propagating through circum-nuclear medium of the AGN.

Dates et versions

hal-03098824 , version 1 (05-01-2021)

Identifiants

Citer

Andrii Neronov, Dmitri Semikoz. Radio-to-Gamma-Ray Synchrotron and Neutrino Emission from Proton–Proton Interactions in Active Galactic Nuclei. JETP Lett., 2021, 113 (2), pp.69-74. ⟨10.1134/S0021364021020028⟩. ⟨hal-03098824⟩
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