# Total Flux of Active ${{\boldsymbol p}}{{\boldsymbol p}}$ Solar Neutrinos INSPIRE search

Total flux of active neutrinos (${{\mathit \nu}_{{e}}},{{\mathit \nu}_{{\mu}}},{{\mathit \nu}_{{\tau}}}$).
VALUE ($10^{10}$ cm${}^{-2}$s${}^{-1}$) DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
$6.1$ $\pm0.5$ ${}^{+0.3}_{-0.5}$ 1
 2018 B
BORX Use ${{\mathit \nu}_{{e}}}{{\mathit e}}$ scattering rate
1  AGOSTINI 2018B obtained this result from the measured ${{\mathit \nu}_{{e}}}{{\mathit e}}$ elastic scattering rate over the period between December 2011 and May 2016, assuming the MSW-LMA oscillation parameters derived by ESTEBAN 2017 . Assuming a high-metalicity standard solar model, the electron neutrino survival probability for the ${{\mathit p}}{{\mathit p}}$ solar neutrino is calculated to be $0.57$ $\pm0.09$.
References:
 AGOSTINI 2018B
NAT 562 505 Comprehensive measurement of $pp$-chain solar neutrinos