Search results for "Oscillation"

showing 10 items of 1257 documents

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 cosmology and Planck

2014

Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmological observables. We summarize the main aspects of cosmological neutrinos and describe how the precision of present cosmological data can be used to learn about neutrino properties. In particular, we discuss how cosmology provides information on the absolute scale of neutrino masses, complementary to beta decay and neutrinoless double-beta decay experiments. We explain why the combination of Planck temperature data with measurements of the baryon acoustic oscillation angular scale provides a strong bound on the sum of neutrino masses, 0.23 eV at the 95% confidence level, while the lensing …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologydark matterHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)PlanckAbsolute scaleParticle Physics - PhenomenologyPhysicsOscillationneutrino massesHigh Energy Physics::PhenomenologyFísicaObservablePlanck temperatureBaryonHigh Energy Physics - Phenomenology13. Climate action[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]symbolsHigh Energy Physics::ExperimentNeutrinocosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector.

2009

A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live-time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the WIMP-proton cross-sections for WIMP masses in the range 250 - 5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences7. Clean energyNuclear physicsWIMP0103 physical sciencesddc:550010306 general physicsNeutrino oscillationNeutrino TelescopeHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonAnnihilation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNeutrino detector13. Climate actionNeutralinoHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical review letters
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Constraining the cosmic radiation density due to lepton number with Big Bang Nucleosynthesis

2011

The cosmic energy density in the form of radiation before and during Big Bang Nucleosynthesis (BBN) is typically parameterized in terms of the effective number of neutrinos N_eff. This quantity, in case of no extra degrees of freedom, depends upon the chemical potential and the temperature characterizing the three active neutrino distributions, as well as by their possible non-thermal features. In the present analysis we determine the upper bounds that BBN places on N_eff from primordial neutrino--antineutrino asymmetries, with a careful treatment of the dynamics of neutrino oscillations. We consider quite a wide range for the total lepton number in the neutrino sector, eta_nu= eta_{nu_e}+e…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectFOS: Physical sciences01 natural sciences7. Clean energysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisNucleosynthesis0103 physical sciencesPlanck010306 general physicsNeutrino oscillationmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and AstrophysicsLepton numberUniverseHigh Energy Physics - PhenomenologysymbolsHigh Energy Physics::ExperimentNeutrinoElectron neutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam

2011

The T2K experiment observes indications of $\nu_\mu\rightarrow \nu_e$ appearance in data accumulated with $1.43\times10^{20}$ protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with $|\Delta m_{23}^2|=2.4\times10^{-3}$ eV$^2$, $\sin^2 2\theta_{23}=1$ and $\sin^2 2\theta_{13}=0$, the expected number of such events is 1.5$\pm$0.3(syst.). Under this hypothesis, the probability to observe six or more candidate events is 7$\times10^{-3}$, equivalent to 2.5$\sigma$ significance. At 90% C.L., the data are consistent with 0.03(0.04)$<\sin^2 2\theta_{13}<$ 0.28(0.34) for $\delta_{\rm CP}=0$ and a normal (inverted) hierarchy.

Particle physicsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2CHOOZ01 natural sciencesParticle identificationHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)neutrino14.60.Pq 13.15.+g 25.30.Pt 95.55.Vj0103 physical sciencesneutrino oscillationMuon neutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSPhysicsNOνATribimaximal mixinghep-ex010308 nuclear & particles physicsT2K experimentFísicaT2K Collaborationparticle identificationElectron neutrinoexperimental resultsPhysical Review Letters
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Combined Analysis of Neutrino and Antineutrino Oscillations at T2K.

2017

T2K reports its first results in the search for CP violation in neutrino oscillations using appearance and disappearance channels for neutrino- and antineutrino-mode beams. The data include all runs from January 2010 to May 2016 and comprise 7.482 ×10^(20) protons on target in neutrino mode, which yielded in the far detector 32 e-like and 135 μ-like events, and 7.471 × 10^(20) protons on target in antineutrino mode, which yielded 4 e-like and 66 μ-like events. Reactor measurements of sin(2)2θ(13) have been used as an additional constraint. The one-dimensional confidence interval at 90% for the phase δCP spans the range (−3.13, −0.39) for normal mass ordering. The CP conservation hypothesis …

Particle physicsGeneral PhysicsNeutrino oscillations; CP violation; Neutrino detectors530 PhysicsPhysics MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences7. Clean energy09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino detectors010306 general physicsNeutrino oscillationGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)01 Mathematical SciencesComputingMilieux_MISCELLANEOUSQCPhysicsScience & Technology02 Physical Sciences010308 nuclear & particles physicshep-exNeutrino oscillationsPhysicsCP violationNeutrino detectorantineutrino oscillationsT2K CollaborationPhysical SciencesCP violationNeutrinoPhysical review letters
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Precise measurement of the neutrino mixing parameter θ23 from muon neutrino disappearance in an off-axis beam

2014

New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57 x 10^{20} protons on target, T2K has fit the energy-dependent nu_mu oscillation probability to determine oscillation parameters. Marginalizing over the values of other oscillation parameters yields sin^2 (theta_{23}) = 0.514 +0.055/-0.056 (0.511 +- 0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Delta m^2_{32} = (2.51 +- 0.10) x 10^{-3} eV^2/c^4 (inverted hierarchy: Delta m^2_{13} = (2.48 +- 0.10) …

Particle physicsGeneral PhysicsPhysics MultidisciplinaryMODELSGeneral Physics and AstronomyFOS: Physical sciencesMASS01 natural sciences09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGMuon neutrino010306 general physicsNeutrino oscillationDETECTORMixing (physics)01 Mathematical SciencesPhysicsNeutronsScience & Technology02 Physical Sciences010308 nuclear & particles physicsScatteringOscillationhep-exPhysicsFísicaT2K CollaborationPhysical SciencesSYMMETRIESHigh Energy Physics::ExperimentNeutrinoHigh energy physics Mixing Parameter estimation Parameter extractionConfidence limit Energy dependent Neutrino oscillations Off-axis neutrino beam Oscillation parameters Oscillation probabilities Precise measurements Statistical uncertaintyBeam (structure)Energy (signal processing)
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Search for coherent charged pion production in neutrino-carbon interactions

2005

We report the result from a search for charged-current coherent pion production induced by muon neutrinos with a mean energy of 1.3 GeV. The data are collected with a fully active scintillator detector in the K2K long-baseline neutrino oscillation experiment. No evidence for coherent pion production is observed and an upper limit of $0.60 \times 10^{-2}$ is set on the cross section ratio of coherent pion production to the total charged-current interaction at 90% confidence level. This is the first experimental limit for coherent charged pion production in the energy region of a few GeV.

Particle physicsMesonPhysics::Instrumentation and DetectorsNeutrino-nucleus reactionsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionExperiment-HEP0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentNuclear ExperimentCharged currentPhysicsMuonTamura Norio010308 nuclear & particles physicsNeutrino oscillationsFísica田村 詔生Production (computer science)High Energy Physics::ExperimentNeutrinoLepton
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Measurement of the inclusive $\nu_{\mu}$ charged current cross section on iron and hydrocarbon in the T2K on-axis neutrino beam

2014

We report a measurement of the $\nu_\mu$ inclusive charged current cross sections on iron and hydrocarbon in the T2K on-axis neutrino beam. The measured inclusive charged current cross sections on iron and hydrocarbon averaged over the T2K on-axis flux with a mean neutrino energy of 1.51 GeV are $(1.444\pm0.002(stat.)_{-0.157}^{+0.189}(syst.))\times 10^{-38}\mathrm{cm}^2/\mathrm{nucleon}$, and $(1.379\pm0.009(stat.)_{-0.147}^{+0.178}(syst.))\times 10^{-38}\mathrm{cm}^2/\mathrm{nucleon}$, respectively, and their cross section ratio is $1.047\pm0.007(stat.)\pm0.035(syst.)$. These results agree well with the predictions of the neutrino interaction model, and thus we checked the correct treatme…

Particle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstronomy & Astrophysics7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsCross section (physics)Physics and Astronomy (all)High Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationNuclear ExperimentDETECTORCharged currentMathematical Physicschemistry.chemical_classificationPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsPhysicsT2K experimentFísicaHydrocarbonchemistryPhysical SciencesHigh Energy Physics::ExperimentNuclear and High Energy Physics; Mathematical Physics; Physics and Astronomy (all)NeutrinoNucleon
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Axion cold dark matter: Status after Planck and BICEP2

2014

We investigate the axion dark matter scenario (ADM), in which axions account for all of the dark matter in the Universe, in light of the most recent cosmological data. In particular, we use the Planck temperature data, complemented by WMAP E-polarization measurements, as well as the recent BICEP2 observations of B-modes. Baryon Acoustic Oscillation data, including those from the Baryon Oscillation Spectroscopic Survey, are also considered in the numerical analyses. We find that, in the minimal ADM scenario, the full dataset implies that the axion mass m_a = 82.2 pm 1.1 {\mu}eV (corresponding to the Peccei-Quinn symmetry being broken at a scale f_a = (7.54 pm 0.10)*10^10 GeV), or m_a = 76.6 …

Particle physicsNuclear and High Energy PhysicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)INFLATIONPlanckAxionPhysicsSpectral indexHigh Energy Physics::PhenomenologyFísicaPlanck temperatureINVISIBLE AXIONBARYON ACOUSTIC-OSCILLATIONS; DIGITAL SKY SURVEY; INVISIBLE AXION; COSMOLOGY; INFLATION; DISTANCEBaryonHigh Energy Physics - PhenomenologyCOSMOLOGYDISTANCEsymbolsDark energyAstronomiaDIGITAL SKY SURVEYBARYON ACOUSTIC-OSCILLATIONSAstrophysics - Cosmology and Nongalactic Astrophysics
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