Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days

Abstract

The first results of the solar neutrino flux measurement from Super-Kamiokande are presented. The results shown here are obtained from data taken between the 31st of May, 1996, and the 23rd of June, 1997. Using our measurement of recoil electrons with energies above 6.5 MeV, we infer the total flux of 8B solar neutrinos to be 2.42+-0.06(stat.)+0.10-0.07(syst.)*10^6/cm^2/s. This result is consistent with the Kamiokande measurement and is 36% of the flux predicted by the BP95 solar model. The flux is also measured in 1.5 month subsets and shown to be consistent with a constant rate.

7 pages, 3 figures

Cited by in corpus (444)

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• Seesaw mechanism in three flavors
• Why PeV scale left-right symmetry is a good thing
• Pati-Salam model in curved space-time from square root Lorentz manifold
• $B \to K \etap$ decays in the SM with fourth generation fermions
• Neutrino Oscillations in the Three Flavor Paradigm
• Geometric gravitational origin of neutrino oscillations and mass-energy
• Improving LMA predictions with non standard interactions
• One-loop corrections to light neutrino masses in gauged U(1) extensions of the standard model
• A Minimal See-Saw Model for Hierarchical Neutrino Masses with Large Mixing
• La aventura de la fisica
• Predictive SUSY GUT Model for CP Violation, Fermion Masses and Mixings
• Gauge and Yukawa Unification in SUSY with Bilinearly Broken R-Parity
• Probing the Solar ${}^8$B Neutrino Fog with XENONnT