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Measuring Atmospheric Neutrino Oscillations with Neutrino Telescopes

Ivone F. M. Albuquerque·George F. Smoot
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Abstract

Neutrino telescopes with large detection volumes can demonstrate that the current indications of neutrino oscillation are correct or if a better description can be achieved with non-standard alternatives. Observations of contained muons produced by atmospheric neutrinos can better constrain the allowed region for oscillations or determine the relevant parameters of non-standard models. We analyze the possibility of neutrino telescopes measuring atmospheric neutrino oscillations. We suggest adjustments to improve this potential. An addition of four densely-instrumented strings to the AMANDA II detector makes observations feasible. Such a configuration is competitive with current and proposed experiments.

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Ivone F. M. Albuquerque, George F. Smoot. 2001-03-28. Measuring Atmospheric Neutrino Oscillations with Neutrino Telescopes. https://doi.org/10.1103/physrevd.64.053008

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