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arXiv · hep-ph/9810468

Tau Appearance In Atmospheric Neutrino Interactions

Lawrence J. Hall·Hitoshi Murayama
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Abstract

If the correct interpretation of the Super-Kamiokande atmospheric neutrino data is ν_μ-> ν_τoscillation, the contained data sample should already have more than 10 tau appearance events. We study the challenging task of detecting the tau, focussing on the decay chain τ^\pm -> ρ^\pm -> π^\pm π^0 in events with quasi-elastic tau production. The background level, which is currently quite uncertain because of a lack of relevant neutral current data, can be measured by the near detector in the K2K experiment. Our estimates of the background suggest that it may be possible to detect tau appearance in Super-Kamiokande with 5-10 years of running.

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Lawrence J. Hall, Hitoshi Murayama. 1998-10-24. Tau Appearance In Atmospheric Neutrino Interactions. https://doi.org/10.1016/s0370-2693(99)00951-x

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