Ultra-high energy cosmic neutrinos
H. Athar
Abstract
Several cosmologically distant astrophysical sources may produce ultra-high energy cosmic neutrinos (E > 106 GeV) of all flavors above the atmospheric neutrino background. I study the effects of vacuum neutrino flavor mixing on this cosmic neutrino flux. Prospects for observations of these ultra-high energy cosmic neutrinos in large underwater/ice neutrino telescopes are also briefly discussed.
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