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arxiv 0808.0824 v1 pith:53HZNG5T submitted 2008-08-06 hep-ex

On the Capability Of Super-Kamiokande Detector To Define the Primary Parameters Of Muon And Electron Events

V.I.Galkin (1) , A.M.Anokhina (1) , E.Konishi (2) , A.Misaki (3)((1) Department of Physics , Moscow State University , Russia , (2) Graduate School of Science , Technology
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Hirosaki University Japan (3) Research Institute for Science Engineering Waseda University Japan)
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classification hep-ex
keywords procedureresolutionangulardiscriminationdistributionelectroneventsgeometrical
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We develop a new discrimination procedure for separating electron neutrinos from muon neutrinos, based on detailed simulations carried out with GEANT3.21 and with mean angular distribution functions and their relative fluctuations. Using our procedure we are able to discriminate muons from electrons in Fully Contained Events in Super-Kamioknade Experiment with a probability of error ofless than several %. Also we have checked geometrical resolution on both cases, considering only the ring-like structure of the Cherenkov image and a geometrical reconstruction procedure utilizing the full distribution. Even the methodologically correct approach we have adopted, we cannot reproduce the accuracies for particle discrimination, momentum resolution, interaction vertex location, and angular resolution obtained by the Super-Kamiokande Collaboration.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraints and Projections for Millicharged Dark Matter in the Sun with Water Cherenkov Neutrino Detectors

    hep-ph 2026-06 unverdicted novelty 5.0

    Super-Kamiokande constrains millicharged dark matter at 5-28 GeV for fractional abundance 10^{-4.5}; Hyper-Kamiokande reaches down to 5x10^{-6}.

  2. Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun

    astro-ph.HE 2025-01 unverdicted novelty 5.0

    Super-Kamiokande data constrains the DM-electron scattering cross-section for leptophilic dark matter to ~4e-41 cm2 below 100 GeV, exceeding direct detection by over an order of magnitude.