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Tau neutrinos interacting inside the Earth produce leptons which thereafter can decay inside the atmosphere. The propagation of extremely energetic \nut’s and ’s through the Earth is studied by means of a detailed Monte Carlo simulation, taking into account all major mechanisms of \nut interactions and energy loss as well as decay modes. The rates of ’s emerging from the Earth are determined as a function of ’s energy for several cosmic neutrino models.

生成讲解博客的中文版本

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