Search results for " Neutrino"

showing 10 items of 727 documents

NuSTEC White Paper: Status and challenges of neutrino–nucleus scattering

2018

International audience; The precise measurement of neutrino properties is among the highest priorities in fundamental particle physics, involving many experiments worldwide. Since the experiments rely on the interactions of neutrinos with bound nucleons inside atomic nuclei, the planned advances in the scope and precision of these experiments require a commensurate effort in the understanding and modeling of the hadronic and nuclear physics of these interactions, which is incorporated as a nuclear model in neutrino event generators. This model is essential to every phase of experimental analyses and its theoretical uncertainties play an important role in interpreting every result.In this Wh…

electron nucleus: interactionNuclear TheoryElementary particle7. Clean energy01 natural sciencesCROSS-SECTIONSScatteringHigh Energy Physics - Phenomenology (hep-ph)Nuclear Experimentneutrino: interactionCOHERENT PION-PRODUCTIONPhysicsstrong interactionElectroweak interactionModel; Neutrino; Nuclear; Nucleus; Oscillations; Scattering; Nuclear and High Energy PhysicsHigh Energy Physics - PhenomenologyMUON-NEUTRINONeutrinoNucleonnumerical calculations: Monte CarloNuclear and High Energy PhysicsParticle physicsOscillationsFORM-FACTORSProcess (engineering)FOS: Physical sciencesELECTROMAGNETIC RESPONSEnuclear modelNucleusMESON-EXCHANGE CURRENTSNNLO QCD ANALYSISCHARGED-CURRENT INTERACTIONSnuclear physicsdeep inelastic scattering0103 physical sciencesNeutrinoNuclear010306 general physicsneutrino nucleus: scatteringresonance: modelelectroweak interaction010308 nuclear & particles physicsR=SIGMA-L/SIGMA-Tneutrino nucleus: interactionDeep inelastic scatteringPhysics and Astronomy13. Climate actionINELASTIC ELECTRON-SCATTERING[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Atomic nucleusneutrino: oscillationEvent (particle physics)Model
researchProduct

Solar neutrino physics with Borexino

2018

We present the most recent solar neutrino results from the Borexino experiment at the Gran Sasso underground laboratory. In particular, refined measurements of all neutrinos produced in the {\it pp} fusion chain have been made. It is the first time that the same detector measures the entire range of solar neutrinos at once. These new data weakly favor a high-metallicity Sun. Prospects for measuring CNO solar neutrinos are also discussed.

fusionPhysics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Astrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear physics0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)Nuclear Experiment010303 astronomy & astrophysicsBorexinoPhysicsp p: fusion010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Gran Sasso* Automatic Keywords *Physics::Space PhysicsUnderground laboratoryBorexinoHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoexperimental resultsSciPost Physics Proceedings
researchProduct

Recent results from Borexino and the first real time measure of solar pp neutrinos

2014

International audience; The Borexino detector was built starting from 1996 in the underground hall C of Gran Sasso National Laboratory (LNGS) in Italy under about 1400 m of rock (3800 m.w.e) and it is mostly aimed to the study in real-time of the low-energy solar neutrinos.Since the beginning of data taking, in May 2007, the unprecedented detector radio-purity made the performances of the detector unique: a milestone has been very recently achieved with the measurement of solar pp neutrino flux, providing the first direct observation in real time of the key fusion reaction powering the Sun.In this contribution the most important Borexino achievements to the fields of solar, geo-neutrino and…

geo-neutrinosNuclear and High Energy PhysicsParticle physicsNeutrino oscillationneutrino: solarPhysics::Instrumentation and DetectorsGeo-neutrinos; Neutrino oscillations; Solar neutrinos; Nuclear and High Energy PhysicsSolar neutrinotalk: Valencia 2014/07/02Solar neutrinosSolar neutrino01 natural sciences7. Clean energyPhysics::Geophysics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530010306 general physicsNeutrino oscillationBorexinoPhysicsneutrino oscillations010308 nuclear & particles physicsNeutrino oscillationsSolar neutrino problemGran SassoNeutrino detectorGeo-neutrinosolar neutrinosMeasurements of neutrino speedBorexinoHigh Energy Physics::Experimentneutrino: oscillationneutrino: geophysicsNeutrino astronomyNeutrinoexperimental resultsGeo-neutrinosNuclear and Particle Physics Proceedings
researchProduct

Review of Particle Physics

2020

The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, …

high energyleptonmixing [neutrino]High Energy Physics::LatticeCosmic microwave backgrounddiffractionTechnicolorAstrophysicsOmega01 natural sciencesPhysics Particles & Fieldshiggs-boson productionBig Bang nucleosynthesiscosmological model: parameter spacetaudark energyMonte CarlofieldspentaquarkinstrumentationSettore FIS/01gauge bosonAnomalous magnetic dipole momentdeep-inelastic scatteringnew physicsPhysicsDOUBLE-BETA-DECAYElectroweak interactiondensity [dark matter]HEAVY FLAVOURQuarkoniumreview; particle; physicsSUPERSYMMETRIC STANDARD MODELsquare-root-sPhysics Nucleargrand unified theoryboson: heavystatisticsPhysical SciencesHiggs bosonaxion: massflavor: violationNeutrinoELECTROWEAK SYMMETRY-BREAKINGnumerical calculations: Monte Carlophysicson-lineS013EPHQuarkheavy [boson]particle[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Physics Multidisciplinaryanomalous magnetic-momentelectroweak radiative-correctionsdark matter: densityHiggs particlemesonneutrino masses neutrino mixing; neutrino oscillations114 Physical sciencesCHIRAL PERTURBATION-THEORYneutrino mixingStandard Modelquark0202 Atomic Molecular Nuclear Particle And Plasma PhysicsNucleosynthesisquantum chromodynamicsCP: violationDark matterddc:530particle physicsStrong Interactions010306 general physicssparticleS013DFgrand unified theoriesPRODUCTIONGauge bosonScience & Technologyneutrino oscillationsneutrino masses010308 nuclear & particles physicsC50 Other topics in experimental particle physicsParticle Data GroupAstronomy and AstrophysicsDeep inelastic scatteringto-leading-order* Automatic Keywords *heavy bosonaxiontables (particle physics)Tetraquarkproton-proton collisionsSupersymmetryhadronneutrino: mixing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyVolume (compression)HIGGS-BOSONUB-VERTICAL-BARcosmological modeldark energy densityexperimental methodsddc:539.72021Physics beyond the Standard Modelstandard modelgroup theoryGeneral Physics and Astronomytables particle physicshigh energy physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamicsPhysicsenergy: highE Rev 2016[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Settore FIS/01 - Fisica SperimentalephotonSupersymmetryNuclear & Particles Physicsparameter space [cosmological model]dark energy: densityhigh [energy]M013WXfermion-pair productionNuclear and High Energy PhysicsParticle physicsHiggs bosonreviewAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics530dark matterstatistical analysisDouble beta decay0103 physical sciencesconservation lawcold dark-matterTAU LEPTONSAstrophysics::Galaxy AstrophysicstablesDEEP-INELASTIC-SCATTERINGelectroweak interactionHigh Energy Physics::Phenomenology750 GeV diphoton excessPRODUCTION CROSS-SECTIONbaryondensity [dark energy]Physics and AstronomygravitationCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentsupersymmetryMinimal Supersymmetric Standard Model
researchProduct

Measurement of Atmospheric Neutrino Oscillations at 6–56 GeV with IceCube DeepCore

2018

We present a measurement of the atmospheric neutrino oscillation parameters using three years of data from the IceCube Neutrino Observatory. The DeepCore infill array in the center of IceCube enables the detection and reconstruction of neutrinos produced by the interaction of cosmic rays in Earth's atmosphere at energies as low as ∼5 GeV. That energy threshold permits measurements of muon neutrino disappearance, over a range of baselines up to the diameter of the Earth, probing the same range of L/Eν as long-baseline experiments but with substantially higher-energy neutrinos. This analysis uses neutrinos from the full sky with reconstructed energies from 5.6 to 56 GeV. We measure Δm322=2.31…

interaction [cosmic radiation]Physics::Instrumentation and DetectorsSolar neutrinoGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCubeSubatomär fysikHigh Energy Physics - Experiment (hep-ex)ObservatorySubatomic PhysicsTOOLPhysicsoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicsatmosphere [neutrino]threshold [energy]mass difference [neutrino]ddc:observatoryNeutrino detectorPhysique des particules élémentairesAstrophysics::Earth and Planetary AstrophysicsNeutrinoParticle physicscosmic radiation [neutrino]acceleratorAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Physics and Astronomy(all)IceCube Neutrino ObservatoryPhysics and Astronomy (all)0103 physical sciencesneutrino/muddc:530energy: high [neutrino]010306 general physicsNeutrino oscillationAstroparticle physics010308 nuclear & particles physicsICEHigh Energy Physics::PhenomenologyAstronomySolar neutrino problemPhysics and Astronomy13. Climate actionmass [neutrino]High Energy Physics::ExperimentSYSTEMmixing angle [neutrino]experimental resultsPhysical Review Letters
researchProduct

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
researchProduct

Theoretical study of supernova neutrino and antineutrino scattering off the stable cadmium and lead isotopes

2017

In this thesis work, an extensive study of neutrino- and antineutrino-nucleus interactions is performed. The work is focused on supernova-neutrino scattering off the stable cadmium and lead isotopes. The studied nuclei are of interest for the investigations of neutrino-properties and for neutrino-detection experiments. The adopted nuclear-structure models are based on the quasiparticle random-phase approximation (QRPA) and the microscopic quasiparticle- phonon model (MQPM) and the cross-sections calculations are based on the Donnelly-Walecka formalism. The computed cross sections are folded with a two-parameter Fermi-Dirac distribution to obtain realistic estimates of the nuclear responses …

leadisotoopitcadmiumAstrophysics::High Energy Astrophysical PhenomenaNuclear Theoryscatteringneutriinotstable isotopesneutrinosnucleisirontalyijyNuclear Experimentsupernova neutrinoskadmium
researchProduct

LeptoGen-koodi

2021

LeptoGen is a software package for numerically solving (resonant) leptogenesis equations including full flavour coherence information for the Majorana neutrinos. The package is written in Wolfram Language and can be run in the Mathematica front end. (Tested in Mathematica 12.0.) For usage license, see the attachment.

leptogeneesileptogenesisparticle physicshiukkasfysiikkacosmologyMajorana neutrinos
researchProduct

Searches for lepton number violation and resonances in K± → πμμ decays

2017

The NA48/2 experiment at CERN collected a large sample of charged kaon decays to final states with multiple charged particles in 2003–2004. A new upper limit on the rate of the lepton number violating decay K±→π∓μ±μ± is reported: B(K±→π∓μ±μ±)<8.6×10−11 at 90% CL. Searches for two-body resonances X in K±→πμμ decays (such as heavy neutral leptons N4 and inflatons χ ) are also presented. In the absence of signals, upper limits are set on the products of branching fractions B(K±→μ±N4)B(N4→πμ) and B(K±→π±X)B(X→μ+μ−) for ranges of assumed resonance masses and lifetimes. The limits are in the (10−11,10−9) range for resonance lifetimes below 100 ps.

leptonBEAM01 natural sciences7. Clean energyPhysics Particles & FieldsHigh Energy Physics - ExperimentLIMITSkaon physicsCERNIntermediate statelepton number violation neutrinos dark matter kaon physicsPhysicsVMSMLarge Hadron ColliderPhysicsCharge KaonsneutrinosNuclear and High Energy Physics; CERN; leptonsHigh Energy Physics - Experiment; Charge Kaons; Lepton number violationNuclear & Particles PhysicsCharged particlelcsh:QC1-999NEUTRAL HEAVY-LEPTONSPhysics Nuclearlepton number violationPhysical SciencesParticle physicsNuclear and High Energy Physicsleptonskaon decays lepton number violationNuclear and High Energy Physics lepton kaon meson lepton number violation NA48Socio-culturaleAstronomy & AstrophysicsUPPER-BOUNDSdark matterNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciencesDARK-MATTERPARTICLES010306 general physicsScience & Technologykaon decays010308 nuclear & particles physicsBranching fractionResonanceInflatonLepton numberkaon mesonNA48High Energy Physics::Experimentlcsh:PhysicsLepton
researchProduct

LBNO-DEMO (WA105): a large demonstrator of the Liquid Argon double phase TPC

2016

LBNO-DEMO (WA105) is a large demonstrator of the double phase liquid argon TPC intended to develop and test the main elements of the GLACIER-based design for the purpose of scaling it up to the 10–50 kton size needed for Long Baseline Neutrino Oscillation studies. The crucial components of the design are: ultra-high argon purity in non-evacuable tank, long drifts, very high drift voltages, large area Micro Pattern Gas Detectors, and cold preamplifiers. The active volume of the demonstrator is 6×6×6 m3 (approximately 300t). WA105 is under construction at CERN and will be exposed to charged particle beams (0.5-20 GeV/c) in the North Area in 2018. The data will provide the necessary calibratio…

liguid argonPhysics::Instrumentation and DetectorsHigh Energy Physics::Experimentlong baseline neutrinostime projection chamber
researchProduct