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      Indications of negative evolution for the sources of the highest energy cosmic rays

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      Physical Review D
      American Physical Society (APS)

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          Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

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            Cosmic rays at ultra high energies (neutrino?)

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              Monte Carlo treatment of hadronic interactions in enhanced Pomeron scheme: QGSJET-II model

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                Author and article information

                Journal
                PRVDAQ
                Physical Review D
                Phys. Rev. D
                American Physical Society (APS)
                1550-7998
                1550-2368
                September 2015
                September 14 2015
                : 92
                : 6
                Article
                10.1103/PhysRevD.92.063011
                63d8093e-cb77-4711-96c4-fb098b6f4c5a
                © 2015

                https://link.aps.org/licenses/aps-default-license

                https://link.aps.org/licenses/aps-default-accepted-manuscript-license

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