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- W3100558240 abstract "Cosmic-ray (CR) acceleration at the shock created by the expanding cocoons around active galactic nuclei (AGNs) is studied. It is shown that above the energy 1018 eV the overall energy spectrum of CRs, produced during the AGN evolution and released in the intergalactic space, has the form N ∝ −γ, with γ ≈ 2.6, which extends up to max ∼ 1020 eV. It is concluded that cocoons shocks have to be considered as a main source of extragalactic CRs, which together with Galactic supernova remnants provide the observed CR spectrum." @default.
- W3100558240 created "2020-11-23" @default.
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- W3100558240 date "2008-08-21" @default.
- W3100558240 modified "2023-09-26" @default.
- W3100558240 title "Cosmic Rays from Active Galactic Nuclei" @default.
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- W3100558240 doi "https://doi.org/10.1086/592233" @default.
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