0000000000349811

AUTHOR

Al. Ianni

showing 2 related works from this author

First real–time detection of solar pp neutrinos by Borexino

2014

International audience; Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the keystone pp reaction, in which two protons fuse to make a deuteron, have so far eluded direct detection. The Borexino experiment, an ultra-pure liquid scintillator detector running at the Laboratori Nazionali del Gran Sasso in Italy, has now filled the gap, providing the first direct real time measurement of pp neutrinos and of the solar neutrino luminosity.

deuteronParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidgap7. Clean energy01 natural sciencesNuclear physicsPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530flavor: oscillation010306 general physicsNuclear ExperimentBorexinoPhysicsICARUSp p: fusion010308 nuclear & particles physicsPhysicsHigh Energy Physics::Phenomenologytalk: Noto 2014/09/30Solar neutrino problemGran SassoNeutrino detectorneutrino: flavorMeasurements of neutrino speedCOUNTING TEST FACILITYHigh Energy Physics::Experimentdirect detectionBorexinoneutrino: oscillationNeutrino astronomyNeutrinoexperimental resultsneutrino: luminosity
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Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

2014

The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as we…

Nuclear reactionPhysics - Instrumentation and DetectorsProtonneutrino: solarPhysics::Instrumentation and Detectors01 natural sciences7. Clean energynuclear reactionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)PositronstarPrimary (astronomy)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysicsSPECTROSCOPYInstrumentation and Detectors (physics.ins-det)SOLAR NEUTRINOSAstrophysics - Solar and Stellar AstrophysicsBorexinoNeutrinomodel: solardeuteronGRAN SASSOParticle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]talk: Conca Specchiulla 2014/09/07[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationDETECTORSolar and Stellar Astrophysics (astro-ph.SR)neutrino: modelp p: fusion010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDeuterium13. Climate actionspectralHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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