Status of direct determination of solar neutrino fluxes after Borexino

Abstract We determine the solar neutrino fluxes from the global analysis of the most up-to-date terrestrial and solar neutrino data including the final results of the three phases of Borexino. The analysis are performed in the framework of three-neutrino mixing with and without accounting for the so...

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Main Authors: M. C. Gonzalez-Garcia, Michele Maltoni, João Paulo Pinheiro, Aldo M. Serenelli
Format: Article
Language:English
Published: SpringerOpen 2024-02-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP02(2024)064
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author M. C. Gonzalez-Garcia
Michele Maltoni
João Paulo Pinheiro
Aldo M. Serenelli
author_facet M. C. Gonzalez-Garcia
Michele Maltoni
João Paulo Pinheiro
Aldo M. Serenelli
author_sort M. C. Gonzalez-Garcia
collection DOAJ
description Abstract We determine the solar neutrino fluxes from the global analysis of the most up-to-date terrestrial and solar neutrino data including the final results of the three phases of Borexino. The analysis are performed in the framework of three-neutrino mixing with and without accounting for the solar luminosity constraint. We discuss the independence of the results on the input from the Gallium experiments. The determined fluxes are then compared with the predictions provided by the latest Standard Solar Models. We quantify the dependence of the model comparison with the assumptions about the normalization of the solar neutrino fluxes produced in the CNO-cycle as well as on the particular set of fluxes employed for the model testing.
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spelling doaj.art-4f0f796afb9f4d3bb5cc0cad517303ab2024-03-05T17:28:17ZengSpringerOpenJournal of High Energy Physics1029-84792024-02-012024213310.1007/JHEP02(2024)064Status of direct determination of solar neutrino fluxes after BorexinoM. C. Gonzalez-Garcia0Michele Maltoni1João Paulo Pinheiro2Aldo M. Serenelli3Departament de Física Quàntica i Astrofísica and Institut de Ciències del Cosmos, Universitat de BarcelonaInstituto de Física Teórica (IFT-CFTMAT), CSIC-UAMDepartament de Física Quàntica i Astrofísica and Institut de Ciències del Cosmos, Universitat de BarcelonaInstitute of Space Sciences (ICE, CSIC)Abstract We determine the solar neutrino fluxes from the global analysis of the most up-to-date terrestrial and solar neutrino data including the final results of the three phases of Borexino. The analysis are performed in the framework of three-neutrino mixing with and without accounting for the solar luminosity constraint. We discuss the independence of the results on the input from the Gallium experiments. The determined fluxes are then compared with the predictions provided by the latest Standard Solar Models. We quantify the dependence of the model comparison with the assumptions about the normalization of the solar neutrino fluxes produced in the CNO-cycle as well as on the particular set of fluxes employed for the model testing.https://doi.org/10.1007/JHEP02(2024)064Neutrino InteractionsNeutrino Mixing
spellingShingle M. C. Gonzalez-Garcia
Michele Maltoni
João Paulo Pinheiro
Aldo M. Serenelli
Status of direct determination of solar neutrino fluxes after Borexino
Journal of High Energy Physics
Neutrino Interactions
Neutrino Mixing
title Status of direct determination of solar neutrino fluxes after Borexino
title_full Status of direct determination of solar neutrino fluxes after Borexino
title_fullStr Status of direct determination of solar neutrino fluxes after Borexino
title_full_unstemmed Status of direct determination of solar neutrino fluxes after Borexino
title_short Status of direct determination of solar neutrino fluxes after Borexino
title_sort status of direct determination of solar neutrino fluxes after borexino
topic Neutrino Interactions
Neutrino Mixing
url https://doi.org/10.1007/JHEP02(2024)064
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