(A) Neutrino fluxes and event ratios

$\phi _{\mathit ES}$ (${}^{7}\mathrm {Be}$)

${}^{7}\mathrm {Be}$ solar-neutrino flux measured via ${{\mathit \nu}_{{e}}}$ elastic scattering. This process is sensitive to all active neutrino flavors, but with reduced sensitivity to ${{\mathit \nu}_{{\mu}}}$ , ${{\mathit \nu}_{{\tau}}}$ due to the cross-section difference, $\sigma\mathrm {( {{\mathit \nu}} _{{{\mathit \mu}} , {{\mathit \tau}} } {{\mathit e}} )}$ $\sim{}0.2$ $\sigma\mathrm {( {{\mathit \nu}_{{e}}} {{\mathit e}} )}$. If the ${}^{7}\mathrm {Be}$ solar-neutrino flux involves nonelectron flavor active neutrinos, their contribution to the flux is $\sim{}0.2$ times that of ${{\mathit \nu}_{{e}}}$ .

VALUE ($ 10^{9} $ cm${}^{-2}$ s${}^{-1}$) DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
$3.26$ $\pm0.52$ 1
KLND average flux
$3.10$ $\pm0.15$ 2
BORX average flux
1  GANDO 2015 uses 165.4 kton$\cdot{}$day exposure of the KamLAND liquid scintillator detector to measure the 862 keV ${}^{7}\mathrm {Be}$ solar neutrino flux via ${{\mathit \nu}}$ $−{{\mathit e}}$ elastic scattering
2  BELLINI 2011A reports the ${}^{7}\mathrm {Be}$ solar neutrino flux measured via ${{\mathit \nu}}$ $−{{\mathit e}}$ elastic scattering. The data correspond to 740.7 live days between May 16, 2007 and May 8, 2010, and also correspond to 153.6 ton$\cdot{}$year fiducial exposure. BELLINI 2011A measured the 862 keV ${}^{7}\mathrm {Be}$ solar neutrino flux, which is an 89.6$\%$ branch of the ${}^{7}\mathrm {Be}$ solar neutrino flux, to be ($27.8$ $\pm1.3$) $ \times 10^{8}$ cm${}^{-2}~$s${}^{-1}$. Supercedes ARPESELLA 2008A.
GANDO 2015
PR C92 055808 ${}^{7}\mathrm {Be}$ Solar Neutrino Measurement with KamLAND
PRL 107 141302 Precision Measurement of the ${}^{7}\mathrm {Be}$ Solar Neutrino Interaction Rate in Borexino