arXiv Analytics

Sign in

arXiv:hep-ph/9812249AbstractReferencesReviewsResources

Solar Neutrino Oscillation Diagnostics at Superkamiokande and Sno

Debasish Majumdar, Amitava Raychaudhuri

Published 1998-12-04Version 1

Results for solar neutrino detection from the SuperKamiokande collaboration have been presented recently while those from the Sudbury Neutrino Observatory are expected in the near future. These experiments are sensitive to the 8B neutrinos from the sun, the shape of whose spectrum is well-known but the normalisation is less certain. We propose several variables, insensitive to the absolute flux of the incident beam, which probe the shape of the observed spectrum and can sensitively signal neutrino oscillations. They provide methods to extract the neutrino mixing angle and mass splitting from the data and also to distinguish oscillation to sequential neutrinos from those to a sterile neutrino.

Related articles: Most relevant | Search more
arXiv:hep-ph/9901401 (Published 1999-01-25)
New Variables For Neutrino Oscillation Diagnostics at Superkamiokande and the Sudbury Neutrino Observatory
arXiv:hep-ph/0109275 (Published 2001-09-28)
A few comments after the charged current measurement at the Sudbury Neutrino Observatory
arXiv:hep-ph/9806311 (Published 1998-06-08)
Mass signature of supernova $ν_μ$ and $ν_τ$ neutrinos in the Sudbury Neutrino Observatory