Abstract
We suggest an experimental measurement that could detect the appearance of tau neutrinos due to νμντ oscillations of atmospheric neutrinos by measuring the energy spectra of neutrino induced showers. τ neutrinos deposit a large fraction of their energy in showers generated by ντ charge current interactions and the subsequent τ-lepton decay. The appearance of ντ will enhance the spectrum of neutrino induced showers in energy ranges corresponding to the neutrino oscillation parameters. A shower rate lower than the “no oscillation” prediction is an indication for νμνs oscillations.
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