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Measurement of CC interactions produced by
8
B solar neutrinos at SNO
SNO Collaboration
Physics
Institute for Gravitation & the Cosmos
Center for Particle and Gravitational Astrophysics
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8
B solar neutrinos at SNO'. Together they form a unique fingerprint.
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Keyphrases
Muon
100%
Sudbury Neutrino Observatory
100%
Solar Neutrinos
100%
Electron Neutrino
100%
Excellent Sensitivity
50%
Angular Distribution
50%
Neutrinos
50%
Electron Scattering
50%
Water Cherenkov Detector
50%
Scattering Measurements
50%
Deuterium
50%
Neutrino Flux
50%
Atmospheric Neutrinos
50%
Ontario Canada
50%
Neutrino Oscillations
50%
Energy Threshold
50%
Supernova Neutrinos
50%
Heavy Water
50%
Charged Current Interactions
50%
Electron Kinetic Energy
50%
Super-Kamiokande
50%
Physics
Solar Electron
100%
Heavy Water
50%