On the Mass Eigenstate Composition of the 8B Neutrinos from the Sun
arXiv:hep-ph/0608149 · doi:10.1088/1475-7516/2007/04/002
Abstract
The present data of gallium experiments provide indirectly the only experimental limit on the fraction of mass eigenstate for the B neutrinos from the Sun. However, if to use the experimental data alone, the fraction of and, consequently, still is allowed to be varied within a rather broad range. The further experimental efforts are needed to clear this point.
13 pages, 1 figure, 1 table. Corrected version, published in JCAP04(2007)002
References in corpus (11)
- Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion
- A Measurement of Atmospheric Neutrino Oscillation Parameters by Super-Kamiokande I
- Electron Energy Spectra, Fluxes, and Day-Night Asymmetries of B Solar Neutrinos from the 391-Day Salt Phase SNO Data Set
- Complete results for five years of GNO solar neutrino observations
- Global analysis of three-flavor neutrino masses and mixings
- 10,000 Standard Solar Models: a Monte Carlo Simulation
- Reactor Measurement of theta_12; Principles, Accuracies and Physics Potentials
- What Fraction of Boron-8 Solar Neutrinos arrive at the Earth as a nu_2 mass eigenstate?
- Solar Neutrino Oscillation Parameters in Experiments with Reactor Anti-Neutrinos
- On the Mass Eigenstate Purity of B^8 Solar Neutrinos
- A Lithium Experiment in the Program of Solar Neutrino Research