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- W2072628650 abstract "As ultra-high energy cosmic ray protons propagate through the universe, they undergo photo-meson interactions with the cosmic microwave background, generating the `cosmogenic' neutrino flux. If a substantial fraction of the cosmic ray primaries are heavy nuclei rather than protons, however, they would preferentially lose energy through photo-disintegration, so the corresponding neutrino flux may be substantially depleted. We investigate this issue using a Monte Carlo simulation of cosmic ray propagation through interagalactic radiation fields and assess the impact of the altered neutrino fluxes on next generation neutrino telescopes." @default.
- W2072628650 created "2016-06-24" @default.
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- W2072628650 date "2005-02-01" @default.
- W2072628650 modified "2023-10-17" @default.
- W2072628650 title "The impact of heavy nuclei on the cosmogenic neutrino flux" @default.
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- W2072628650 doi "https://doi.org/10.1016/j.astropartphys.2004.11.002" @default.
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