Astrophysical upper bounds on neutrino-nucleon cross-section at energy E >= 3 × 1017 eV

Physics

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Scientific paper

The possibility of experiments with cosmic neutrinos of energy E > 3
× 1017 eV is discussed. The upper bound of
neutrino-nucleon cross-section σ < 9.3 × 10-30
cm2 is obtained from the zenith angular distribution of
extensive air showers under some particular astrophysical assumptions.

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