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I discuss the possibility of production of high energy cosmic tau neutrinos ( 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 km surface area under water/ice neutrino telescopes.

生成讲解博客的中文版本

生成AI智能校验的中文版本