Neutrino Mixing - Particle Data Group - CERN

Citation: K. Nakamura et al. (Particle Data Group), JP G 37, 075021 (2010) and 2011 partial update for the 2012 edition (URL: http://pdg.lbl.gov)
φ CC(pp) CC(pp)
pp solar-neutrino flux measured with charged-current reaction which is sensitive exclusively
to ν e .
VALUE (10 10 cm −2 s −1 ) DOCUMENT ID TECN COMMENT
•••We do not use the following data for averages, fits, limits, etc. •••
3.38±0.47 1 ABDURASHI... 09 FIT Fit existing solar-ν data
1 ABDURASHITOV 09 reports the pp solar-neutrino flux derived from the Ga solar neutrino
capture rate by subtracting contributions from 8B, 7Be, pep and CNO solar neutrino
fluxes determined by other solar neutrino experiments as well as neutrino oscillation
parameters determined from available world neutrino oscillation data.
φ φ ES (hep)
hep solar-neutrino flux measured via ν e elastic scattering. This process is sensitive
to all active neutrino flavors, but with reduced sensitivity to ν μ , ν τ due to the crosssection
difference, σ(ν μ,τ e) ∼ 0.16σ(ν e e). If the hep solar-neutrino flux involves
nonelectron flavor active neutrinos, their contribution to the flux is ∼ 0.16 times of
ν e .
VALUE (10 3 cm −2 s −1 ) CL% DOCUMENT ID TECN
•••We do not use the following data for averages, fits, limits, etc. •••