High Energy Cosmic Tau Neutrinos
Abstract
I discuss the possibility of production of high energy cosmic tau neutrinos (E ≥ 106 GeV) in an astrophysical site and study some of the effects of neutrino mixing on their subsequent propagation. I also discuss the prospects for observations of these high energy cosmic tau neutrinos through double shower events in new km2 surface area under water/ice neutrino telescopes.
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