Abstract
We present the simultaneous measurement of the interaction rates , , of , , and solar neutrinos performed with a global fit to the Borexino data in an extended energy range (0.19–2.93) MeV with particular attention to details of the analysis methods. This result was obtained by analyzing 1291.51 days of Borexino Phase-II data, collected after an extensive scintillator purification campaign. Using counts per day as unit, we find , ; and assuming the interaction rate of CNO-cycle (Carbon, Nitrogen, Oxigen) solar neutrinos according to the prediction of the high metallicity standard solar model, and according to that of the low metallicity model. An upper limit (95% C.L.) is obtained by setting in the fit a constraint on the ratio ( or according to the high or low metallicity hypothesis).
4 More- Received 6 May 2019
DOI:https://doi.org/10.1103/PhysRevD.100.082004
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Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society