Measuring Atmospheric Neutrino Oscillations with Neutrino Telescopes

Details Measuring Atmospheric Neutrino Oscillations with Neutrino Telescopes Measuring Atmospheric Neutrino Oscillations with Neutrino Telescopes

2001-02-07

arxiv.org/abs/hep-ph/0102078v2

Phys.Rev. D64 (2001) 053008

Physics

High Energy Physics

High Energy Physics - Phenomenology

36 pages, 21 figures, revtex

Scientific paper

10.1103/PhysRevD.64.053008

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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