Ultra High Energy neutrinos detected from the orbit: possibilities, limits and technical problems
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The Double Donut Schmidt Camera for the cosmogenic neutrino detection
2020, Advances in Space ResearchCitation Excerpt :Depending on the assumed hypotheses, the expected cosmogenic neutrino fluxes covered a wide range from a minimum of 100/(eV/cm2s sr) neutrinos from 0.1 to 10 EeV to a maximum of 600/(eV/cm2s sr) from 10 to 1000 EeV. These fluxes were used for the counting rate estimations of the expected cosmogenic neutrino events in the phase A report of EUSO to ESA (EUSO, 2004b; Spillantini et al., 2006). Those previsions were subsequently updated for accounting the new results of Fermi observatory (Ahlers et al., 2010).
A EUSO-like experiment as a precursor of a ultra-high energy neutrino Space Observatory
2018, Nuclear and Particle Physics Proceedings
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