0000000000741444

AUTHOR

O. Yu. Smirnov

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Measurement of Solar pp-neutrino flux with Borexino: results and implications

2015

International audience; Measurement of the Solar pp-neutrino flux completed the measurement of Solar neutrino fluxes from the pp-chain of reactions in Borexino experiment. The result is in agreement with the prediction of the Standard Solar Model and the MSW/LMA oscillation scenario. A comparison of the total neutrino flux from the Sun with Solar luminosity in photons provides a test of the stability of the Sun on the 10(5) years time scale, and sets a strong limit on the power production by the unknown energy sources in the Sun.

model: solarHistoryneutrino: solarSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaluminosity: solarSolar luminosity[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyneutrino: fluxEducationLuminosityNuclear physicsPhysics and Astronomy (all)SEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsDETECTORBorexinoMSW effectPhysicsStandard solar modelSolar energetic particles010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyphotonAstronomySolar neutrino problemstabilityoscillationComputer Science Applicationsp p13. Climate actionPhysics::Space PhysicsBorexinoAstrophysics::Earth and Planetary AstrophysicsNeutrinoexperimental results
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