Search results for "neutrino-nucleus interactions"

showing 5 items of 5 documents

Neutrino-nuclear responses for astro-neutrinos, single beta decays and double beta decays

2019

Abstract Neutrino–nuclear responses associated with astro-neutrinos, single beta decays and double beta decays are crucial in studies of neutrino properties of interest for astro-particle physics. The present report reviews briefly recent studies of the neutrino–nuclear responses from both experimental and theoretical points of view in order to obtain a consistent understanding of the many facets of the neutrino–nuclear responses. Subjects discussed in this review include (i) experimental studies of neutrino–nuclear responses by means of single beta decays, charge-exchange nuclear reactions, muon- photon- and neutrino–nuclear reactions, and nucleon-transfer reactions, (ii) implications of a…

Nuclear reactionParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoastrofysiikkasingle beta decaysNuclear TheoryGeneral Physics and Astronomyneutrino-nucleus interactionsnuclear matrix elements01 natural sciences7. Clean energyastro-neutrinosNucleosynthesisDouble beta decay0103 physical sciencesBeta (velocity)Nuclear Experiment010306 general physicsPhysicsdouble beta decaysMuonta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologymuon captureneutriinotMuon capturephoto-nuclear reactionsHigh Energy Physics::Experimentcharge-exchange reactionsNeutrinoPhysics Reports
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Theoretical estimates of supernova-neutrino cross sections for the stable even-even lead isotopes: Charged-current reactions

2016

A detailed study of the charged-current supernova electron neutrino and electron antineutrino scattering off the stable even-mass lead isotopes $A=204$, 206, and 208 is reported in this work. The proton-neutron quasiparticle random-phase approximation (pnQRPA) is adopted to construct the nuclear final and initial states. Three different Skyrme interactions are tested for their isospin and spin-isospin properties and then applied to produce (anti)neutrino-nucleus scattering cross sections for (anti)neutrino energies below 80 MeV. Realistic estimates of the nuclear responses to supernova (anti)neutrinos are computed by folding the computed cross sections with a two-parameter Fermi-Dirac distr…

Particle physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear Theoryneutrino-nucleus interactionsElectronelectron neutrino01 natural sciencesNuclear physics0103 physical sciencesNuclear Experiment010306 general physicsNeutrino oscillationsupernova neutrinosCharged currentPhysicsta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyscatteringelectron antineutrinoSupernovalead isotopesIsospinQuasiparticleHigh Energy Physics::ExperimentNeutrinoElectron neutrinoPhysical Review C
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Neutrino-nuclear responses for astro-neutrinos, single beta decays and double beta decays

2019

Neutrino–nuclear responses associated with astro-neutrinos, single beta decays and double beta decays are crucial in studies of neutrino properties of interest for astro-particle physics. The present report reviews briefly recent studies of the neutrino–nuclear responses from both experimental and theoretical points of view in order to obtain a consistent understanding of the many facets of the neutrino–nuclear responses. Subjects discussed in this review include (i) experimental studies of neutrino–nuclear responses by means of single beta decays, charge-exchange nuclear reactions, muon- photon- and neutrino–nuclear reactions, and nucleon-transfer reactions, (ii) implications of and discus…

double beta decaysPhysics::Instrumentation and Detectorssingle beta decaysastrofysiikkaHigh Energy Physics::PhenomenologyNuclear Theorymuon captureneutriinotneutrino-nucleus interactionsnuclear matrix elementsastro-neutrinosphoto-nuclear reactionsaxial-vector couplingsolar neutrinosHigh Energy Physics::Experimentcharge-exchange reactionsNuclear Experimentsupernova neutrinos
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The gallium anomaly revisited

2019

The gallium anomaly, i.e. the missing electron-neutrino flux from $^{37}$Ar and $^{51}$Cr electron-capture decays as measured by the GALLEX and SAGE solar-neutrino detectors, has been among us already for about two decades. We present here a new estimate of the significance of this anomaly based on cross-section calculations using nuclear shell-model wave functions obtained by exploiting recently developed two-nucleon interactions. The gallium anomaly of the GALLEX and SAGE experiments is found to be smaller than that obtained in previous evaluations, decreasing the significance from 3.0σ to 2.3σ. This result is compatible with the recent indication in favor of short-baseline ν¯e disappeara…

gallium anomalyNuclear and High Energy PhysicsNuclear Theorychemistry.chemical_elementFluxFOS: Physical sciencesneutrino-nucleus interactions01 natural sciencesNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGallium010306 general physicsWave functionMixing (physics)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNuclear shell modelcharged-current cross-sectionslcsh:QC1-999High Energy Physics - Phenomenologynuclear shell modelchemistryHigh Energy Physics::ExperimentAnomaly (physics)NeutrinoGALLEXydinfysiikkalcsh:PhysicsPhysics Letters B
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Theoretical estimates of supernova-neutrino cross sections for the stable even-even lead isotopes: Charged-current reactions

2016

A detailed study of the charged-current supernova electron neutrino and electron antineutrino scattering off the stable even-mass lead isotopes A = 204, 206, and 208 is reported in this work. The proton-neutron quasiparticle random-phase approximation (pnQRPA) is adopted to construct the nuclear final and initial states. Three different Skyrme interactions are tested for their isospin and spin-isospin properties and then applied to produce (anti)neutrino-nucleus scattering cross sections for (anti)neutrino energies below 80 MeV. Realistic estimates of the nuclear responses to supernova (anti)neutrinos are computed by folding the computed cross sections with a two-parameter Fermi-Dirac distr…

lead isotopesAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNuclear TheoryscatteringHigh Energy Physics::Experimentneutrino-nucleus interactionselectron neutrinoNuclear Experimentelectron antineutrinosupernova neutrinos
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