Search results for "n: semileptonic decay"

showing 2 items of 2 documents

Design of the Magnet System of the Neutron Decay Facility PERC

2018

The PERC (Proton and Electron Radiation Channel) facility is currently under construction at the research reactor FRM II, Garching. It will serve as an intense and clean source of electrons and protons from neutron beta decay for precision studies. It aims to contribute to the determination of the Cabibbo-Kobayashi-Maskawa quark-mixing element $V_{ud}$ from neutron decay data and to search for new physics via new effective couplings. PERC's central component is a 12m long superconducting magnet system. It hosts an 8m long decay region in a uniform field. An additional high-field region selects the phase space of electrons and protons which can reach the detectors and largely improves system…

Physics - Instrumentation and Detectorsmagnet: designProtonQC1-999FOS: Physical sciencesSuperconducting magnetElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyelectron: particle sourcep: particle sourceNuclear physics0103 physical sciencesResearch reactorNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysicsn: semileptonic decay010308 nuclear & particles physicsPhysicsInstrumentation and Detectors (physics.ins-det)magnet: superconductivityMagnetic fieldbeam opticsMagnetPhase spaceHigh Energy Physics::Experiment
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Improved measurement of $^8$B solar neutrinos with $1.5  kt·y$ of Borexino exposure

2017

We report on an improved measurement of the $^8$B solar neutrino interaction rate with the Borexino experiment at the Laboratori Nazionali del Gran Sasso. Neutrinos are detected via their elastic scattering on electrons in a large volume of liquid scintillator. The measured rate of scattered electrons above 3 MeV of energy is $0.223\substack{+0.015 \\ -0.016}\,(stat)\,\substack{+0.006 \\ -0.006}\,(syst)$ cpd/100 t, which corresponds to an observed solar neutrino flux assuming no neutrino flavor conversion of $\Phi\substack{\rm ES \\ ^8\rm B}=2.57\substack{+0.17 \\ -0.18}(stat)\substack{+0.07\\ -0.07}(syst)\times$10$^6$ cm$^{-2}\,$s$^{-1}$. This measurement exploits the active volume of the …

model: solarneutrino: solarPhysics::Instrumentation and Detectorsscintillation counter: liquidFOS: Physical sciencesneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)cosmic raysS067HPT[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Experiments in gravityNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)neutrino: interactionMSW effectcosmic radiation: energy spectrumscintillation counter: targetS067SESneutrino electron: elastic scatteringGran SassoAstrophysics - Solar and Stellar Astrophysicsneutrino: flavorHigh Energy Physics::ExperimentBorexino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyboron: semileptonic decayexperimental results
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