Oscillating atmospheric neutrinos: νμ/μ ratio in surface neutrino telescopes

Details Oscillating atmospheric neutrinos: νμ/μ ratio in surface neutrino telescopes Oscillating atmospheric neutrinos: νμ/μ ratio in surface neutrino telescopes

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..46..505d&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 46, Issue 2, 15 July 1992, pp.505-509

Physics

2

Scientific paper

Surface neutrino telescopes have the capability of detecting neutrinos and muons of similar energy. In a νμ oscillation experiment one can therefore tag the π progenitor of the neutrino by detecting the muon produced in the same decay. This eliminates the model dependence of the measurement inevitably associated with the calculation of the primary-cosmic-ray flux. We show that planned surface neutrino telescopes probe the parameter space Δm2>~10-3 eV2 and sin22θ>~10-3 using this technique.

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