(A) Neutrino fluxes and event ratios

Total Flux of Active CNO Solar Neutrinos

INSPIRE   PDGID:
S067CNT
Total flux of active neutrinos (${{\mathit \nu}_{{e}}},{{\mathit \nu}_{{\mu}}},{{\mathit \nu}_{{\tau}}}$).
VALUE ($ 10^{8} $ cm${}^{-2}$ s${}^{-1}$) CL% DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
$6.6$ ${}^{+2.0}_{-0.9}$ 1
APPEL
2022
BORX ${{\mathit \nu}_{{e}}}{{\mathit e}}$ scattering rate
$7.0$ ${}^{+3.0}_{-2.0}$ 2
AGOSTINI
2020D
 BORX ${{\mathit \nu}_{{e}}}{{\mathit e}}$ scattering rate
$<7.9$ 95 3
AGOSTINI
2018B
 BORX ${{\mathit \nu}_{{e}}}{{\mathit e}}$ scattering rate
1  APPEL 2022 obtained this result from the measured ${{\mathit \nu}_{{e}}}{{\mathit e}}$ elastic scattering rate over the period between January 2017 and October 2021, assuming the MSW-LMA oscillation parameters derived by ESTEBAN 2020A. The exposure corresponding to this data is 1431.6 days ${\times }$ 71.3 tons.
2  AGOSTINI 2020D obtained this result from the measured ${{\mathit \nu}_{{e}}}{{\mathit e}}$ elastic scattering rate over the period between July 2016 to February 2020, assuming the MSW-LMA oscillation parameters derived by CAPOZZI 2018 .
3  AGOSTINI 2018B obtained this result from an upper limit of the ${{\mathit \nu}_{{e}}}{{\mathit e}}$ elastic scattering rate for the CNO neutrinos over the period between December 2011 and May 2016, assuming the MSW-LMA oscillation parameters derived by ESTEBAN 2017 .
References:
APPEL 2022
PRL 129 252701 Improved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model
AGOSTINI 2020D
NAT 587 577 Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun
AGOSTINI 2018B
NAT 562 505 Comprehensive measurement of $pp$-chain solar neutrinos