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• W1974495948 abstract "Although the sources and composition of ultra-high energies cosmic rays is unknown, in most scenarios a significant flux of very high energy neutrinos should be present throughout the universe. We show that even if ultra-high energy cosmic rays are composed of heavy nuclei from extragalactic sources, their propagation over cosmological distances generate a neutrino flux comparable to that of proton primaries depending on the maximum energy and cosmological evolution of the source. The resulting neutrino flux has a new peak at ∼ 1014 eV generated by neutron decay and reproduces the double peak structure due to photopion production at higher energies (∼ 1018 eV). The generated neutrino flux may be detected by future experiments." @default.
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• W1974495948 date "2004-11-01" @default.
• W1974495948 modified "2023-10-18" @default.
• W1974495948 title "Ultra-High Energy Cosmic Rays and Cosmogenic Neutrinos" @default.
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• W1974495948 doi "https://doi.org/10.1016/j.nuclphysbps.2004.10.064" @default.
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