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- W4293491752 abstract "The ultra high energy cosmic neutrinos are powerful astrophysical probes for both astrophysical mechanisms of particle acceleration and fundamental interactions. They open a window into the very distant and high-energy Universe that is difficult to access by any human means and devices. The possibility of detecting them in large exposure space-based apparatus, like JEM-EUSO, is an experimental challenge. In this paper we present an estimation of the feasibility of detection of UHE tau neutrino by the JEM-EUSO telescope. The interactions of tau-neutrino in sea water and Earth's crust have been investigated. The estimation of the propagation length and energy of the outgoing tau-lepton shows that if its decay occurs in the atmosphere close enough to the Earth's surface, e.g. below $sim$ $5 km$ altitude, the cascade is intensive enough and the generated light can be detected from space. We have evaluated the geometrical aperture of the JEM-EUSO detector for the Earth-skimming (horizontal and upward-going) tau-neutrinos by making specific modifications to the standard CORSIKA code and developing an interface to the existing ESAF (EUSO Simulation and Analysis Framework) software." @default.
- W4293491752 created "2022-08-29" @default.
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- W4293491752 date "2015-09-20" @default.
- W4293491752 modified "2023-09-30" @default.
- W4293491752 title "Detection of Earth-skimming UHE tau neutrino with the JEM-EUSO detector" @default.
- W4293491752 doi "https://doi.org/10.48550/arxiv.1509.05995" @default.
- W4293491752 hasPublicationYear "2015" @default.
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