Search results for "NEUTRINO"

showing 10 items of 1752 documents

Determining the nuclear neutron distribution from Coherent Elastic neutrino-Nucleus Scattering: current results and future prospects

2020

Coherent Elastic neutrino-Nucleus Scattering (CEνNS), a process recently measured for the first time at ORNL’s Spallation Neutron Source, is directly sensitive to the weak form factor of the nucleus. The European Spallation Source (ESS), presently under construction, will generate the most intense pulsed neutrino flux suitable for the detection of CEνNS. In this paper we quantify its potential to determine the root mean square radius of the point-neutron distribution, for a variety of target nuclei and a suite of detectors. To put our results in context we also derive, for the first time, a constraint on this parameter from the analysis of the energy and timing data of the CsI detector at t…

Nuclear and High Energy PhysicsField theory (Physics)Nuclear TheoryPhysics::Instrumentation and DetectorsFOS: Physical sciencesContext (language use)01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsRoot mean squareNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutronSpallationNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrinsNuclear Experiment (nucl-ex)Neutrinos010306 general physicsNuclear ExperimentNuclear ExperimentPhysics010308 nuclear & particles physicsScatteringDetectorTeoria de camps (Física)Effective Field TheoriesHigh Energy Physics - Phenomenologylcsh:QC770-798NeutrinoSpallation Neutron Source
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Combining data from high-energy p p -reactions and neutrinoless double-beta decay: Limits on the mass of the right-handed boson

2016

From the recently established lower-limits on the nonobservability of the neutrinoless double-beta decay of 76Ge (GERDA collaboration) and 136Xe (EXO-200 and KamLAND-Zen collaborations), combined with the ATLAS and CMS data, we extract limits for the left-right (LR) mixing angle, of the SU(2)L ×SU(2)R electroweak Hamiltonian. For the theoretical analysis, which is a model dependent, we have adopted a minimal extension of the Standard Model (SM) of Electroweak Interactions belonging to the SU(2)L ×SU(2)R representation. The nuclear-structure input of the analysis consists of a set of matrix elements and phase-space factors, and the experimental lower-limits for the half-lives. The other inpu…

Nuclear and High Energy PhysicsHigh energyParticle physicsCiencias AstronómicasPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelCiencias FísicasGeneral Physics and Astronomy01 natural sciencesRIGHT-HANDED CURRENTS//purl.org/becyt/ford/1 [https]Nuclear physicssymbols.namesakeNEUTRINOLESS DOUBLE-BETA-DECAYDouble beta decay0103 physical sciences010306 general physicsMASS OF THE RIGHT-HANDED BOSONSBosonPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicsAtlas (topology)Electroweak interactionMass of the right-handed bosonsRight-handed currents//purl.org/becyt/ford/1.3 [https]Minimal extension of the standard modelAstronomíasymbolsNeutrinoless double-beta-decayMINIMAL EXTENSION OF THE STANDARD MODELHigh Energy Physics::ExperimentHamiltonian (quantum mechanics)CIENCIAS NATURALES Y EXACTAS
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Measurement of the Inclusive NuMu Charged Current Cross Section on Carbon in the Near Detector of the T2K Experiment

2013

T2K has performed the first measurement of nu(mu) inclusive charged current interactions on carbon at neutrino energies of similar to 1 GeV where the measurement is reported as a flux-averaged double differential cross section in muon momentum and angle. The flux is predicted by the beam Monte Carlo and external data, including the results from the NA61/SHINE experiment. The data used for this measurement were taken in 2010 and 2011, with a total of 10.8 x 10(19) protons-on-target. The analysis is performed on 4485 inclusive charged current interaction candidates selected in the most upstream fine-grained scintillator detector of the near detector. The flux-averaged total cross section is (…

Nuclear and High Energy PhysicsHigher educationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino reactionsLibrary scienceFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyNeutrino scatteringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Early career010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsbusiness.industry4. EducationNuclear TargetsT2K experimentFísicaRussian federationChristian ministryAngular dependenceHigh Energy Physics::Experimentbusiness
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Light Composite Higgs from Higher Representations versus Electroweak Precision Measurements -- Predictions for LHC

2005

We investigate theories in which the technifermions in higher dimensional representations of the technicolor gauge group dynamically break the electroweak symmetry of the standard model. For the two-index symmetric representation of the gauge group the lowest number of techniflavors needed to render the underlying gauge theory quasi conformal is two. We confront the models with the recent electroweak precision measurements and demonstrate that the two technicolor theory is a valid candidate for a dynamical breaking of the electroweak symmetry. The electroweak precision measurements provide useful constraints on the relative mass splitting of the new leptons needed to cure the Witten anomaly…

Nuclear and High Energy PhysicsHyperchargeParticle physicsSterile neutrinoHigh Energy Physics::LatticeFOS: Physical sciencesTechnicolorAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsGauge boson010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)High Energy Physics - Lattice (hep-lat)SupersymmetryHigh Energy Physics - PhenomenologyHiggs bosonHigh Energy Physics::Experiment
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Time projection chambers for the T2K near detectors

2011

The T2K experiment is designed to study neutrino oscillation properties by directing a high intensity neutrino beam produced at J-PARC in Tokai, Japan, towards the large Super-Kamiokande detector located 295 km away, in Kamioka, Japan. The experiment includes a sophisticated near detector complex, 280 m downstream of the neutrino production target in order to measure the properties of the neutrino beam and to better understand neutrino interactions at the energy scale below a few GeV. A key element of the near detectors is the ND280 tracker, consisting of two active scintillator–bar target systems surrounded by three large time projection chambers (TPCs) for charged particle tracking. The d…

Nuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsddc:500.2Tracking (particle physics)01 natural sciences7. Clean energyNuclear physics0103 physical sciences010306 general physicsNeutrino oscillationInstrumentationPhysicsTime projection chamber010308 nuclear & particles physicsDetectorT2K experimentDrift chamber Gas system Micromegas Neutrino oscillation Time projection chamberFísicaMicroMegas detectorTime projectionchamberGas systemCharged particleTime projection chamberDrift chamberHigh Energy Physics::ExperimentNeutrinoMicromegas
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Linear response theory and neutrino mean free path using Brussels-Montreal Skyrme functionals

2014

The Brussels-Montreal Skyrme functionals have been successful in describing properties of both finite nuclei and infinite homogeneous nuclear matter. In their latest version, these functionals have been equipped with two extra density-dependent terms in order to reproduce simultaneously ground state properties of nuclei and infinite nuclear matter properties while avoiding at the same time the arising of ferromagnetic instabilities. In the present article, we extend our previous results of the linear response theory to include such extra terms at both zero and finite temperature in pure neutron matter. The resulting formalism is then applied to derive the neutrino mean free path. The predic…

Nuclear and High Energy PhysicsNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Mean free pathHARTREE-FOCK CALCULATIONSMODELSNuclear TheoryAb initioFOS: Physical sciencesSUSCEPTIBILITYNuclear Theory (nucl-th)Quantum mechanicsNeutronDENSE MATTERCOLDNUCLEAR-MATTERMathematical physicsPhysicsHOTFísicaNuclear matterEQUATION-OF-STATEPhysics and AstronomyHomogeneousNeutrinoGround stateLinear response theoryRPA
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Analysis of the Intermediate-State Contributions to Neutrinoless Double β− Decays

2016

A comprehensive analysis of the structure of the nuclear matrix elements (NMEs) of neutrinoless double beta-minus (0νβ-β-) decays to the0+ground and first excited states is performed in terms of the contributing multipole states in the intermediate nuclei of0νβ-β-transitions. We concentrate on the transitions mediated by the light (l-NMEs) Majorana neutrinos. As nuclear model we use the proton-neutron quasiparticle random-phase approximation (pnQRPA) with a realistic two-nucleon interaction based on the Bonn one-boson-exchangeGmatrix. In the computations we include the appropriate short-range correlations, nucleon form factors, and higher-order nucleonic weak currents and restore the isospi…

Nuclear and High Energy PhysicsParticle physicsArticle SubjectNuclear Theorydouble beta decaynuclear matrix elements01 natural sciencesneutrinoless double beta decayNuclear physicsMatrix (mathematics)0103 physical sciences010306 general physicsNuclear ExperimentPhysicsta114010308 nuclear & particles physicslcsh:QC1-999MAJORANAExcited stateIsospinQuasiparticleNeutrinoMultipole expansionNucleonlcsh:PhysicsAdvances in High Energy Physics
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Charged-current neutrino-nucleus scattering off the even molybdenum isotopes

2012

Neutrinos from supernovae constitute important probes of both the currently unknown supernova mechanisms and of neutrino properties. Reliable information about the nuclear responses to supernova neutrinos is therefore crucial. In this work, we compute the cross sections for the charged-current neutrino-nucleus scattering off the even-even molybdenum isotopes. The nuclear responses to supernova neutrinos are subsequently calculated by folding the cross sections with a Fermi-Dirac distribution.

Nuclear and High Energy PhysicsParticle physicsArticle SubjectPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementAstrophysics::Cosmology and Extragalactic AstrophysicsNuclear physicsmedicineCharged currentPhysicsIsotopeta114ScatteringHigh Energy Physics::Phenomenologylcsh:QC1-999Supernovamedicine.anatomical_structurechemistryTheoretical nuclear physicsMolybdenumteoreettinen ydinfysiikkaHigh Energy Physics::ExperimentNeutrinoNucleuslcsh:PhysicsAdvances in High Energy Physics
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Solar Neutrino Observables Sensitive to Matter Effects

2010

We discuss constraints on the coefficient A_{MSW} which is introduced to simulate the effect of weaker or stronger matter potential for electron neutrinos with the current and future solar neutrino data. The currently available solar neutrino data leads to a bound A_{MSW} = 1.47^{-0.42}_{+0.54} (^{-0.82}_{+1.88}) at 1\sigma (3\sigma) CL, which is consistent with the Standard Model prediction A_{MSW} = 1. For weaker matter potential (A_{MSW} 1), the bound is milder and is dominated by the day-night asymmetry of ^8B neutrino flux recently observed by Super-Kamiokande. Among the list of observable of ongoing and future solar neutrino experiments, we find that (1) an improved precision of the d…

Nuclear and High Energy PhysicsParticle physicsArticle SubjectSolar neutrinomedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences7. Clean energy01 natural sciencesAsymmetryStandard ModelHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationBorexinomedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemlcsh:QC1-999High Energy Physics - Phenomenology13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAdvances in High Energy Physics
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Size of the dark side of the solar neutrino parameter space

2000

We present an analysis of the MSW neutrino oscillation solutions of the solar neutrino problem in the framework of two-neutrino mixing in the enlarged parameter space $(\ensuremath{\Delta}{m}^{2},{\mathrm{tan}}^{2}\ensuremath{\theta})$ with $\ensuremath{\theta}\ensuremath{\in}(0,\ensuremath{\pi}/2).$ Recently, it was pointed out that the allowed region of parameters from a fit to the measured total rates can extend to values $\ensuremath{\theta}g~\ensuremath{\pi}/4$ (the so-called ``dark side'') when higher confidence levels are allowed. The purpose of this Rapid Communication is to reanalyze the problem, including all the solar neutrino data available, to discuss the dependence on the stat…

Nuclear and High Energy PhysicsParticle physicsAstrofísica nuclearElectron energy spectrumSolar neutrinoSolar neutrinosOctant (solid geometry)Parameter spaceEarth-Internal structurePartícules (Física nuclear)Nuclear physicsNeutrins solarsCollisions (Nuclear physics)Resonance oscillationNeutrino oscillationZenithParticles (Nuclear physics)PhysicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemEstructura interna de la terraCol·lisions (Física nuclear)High Energy Physics::ExperimentNuclear astrophysics
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