Search results for "Measurements"

showing 10 items of 720 documents

Neutrino mass and new light gauge boson in superstring models

1987

Abstract The proposal that the neutrino owes the smallness of its mass to the spontaneous breaking of R parity in superstring models with an additional gauge boson coupled to the right-handed neutrino is analysed. The right-handed neutrino can not in general decouple from the low-energy theory in models with supersymmetry at the TeV scale and which possess the light Higgs doublets necessary for generating fermion masses. Experimental limits on neutrino mass then imply an upper limit on the new gauge boson mass m Zr ⪅ 220 GeV.

PhysicsNuclear and High Energy PhysicsGauge bosonSterile neutrinoParticle physicsNeutrino theory of lightAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySupersymmetryHigh Energy Physics::TheoryHiggs bosonMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysics Letters B
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A $B_4C$-silicon target for the detection of neutrino interactions

1998

This note describes the construction of a target for neutrino interactions composed of passive boron carbide plates interleaved with silicon microstrip detectors. The target contains four layers of passive material with a total mass of 45 kg and 600 single--sided silicon microstrip detectors with a total surface of 1.14 m$^2$ distributed over five layers. It is installed in the NOMAD spectrometer at the CERN SPS neutrino beam. During the 1997 run about 8000 \nm\ charged current interactions were estimated to have occurred in the target. For these events it will be possible to perform a precise measurement of both vertex and kinematical variables. This will provide invaluable experience towa…

PhysicsNuclear and High Energy PhysicsLarge Hadron ColliderSpectrometerSiliconPhysics::Instrumentation and DetectorsFísicachemistry.chemical_elementsilicon microstrip detectors; neutrino oscillations; silicon strip sensors; tracking detectors; search; alignmentNuclear physicsNeutrino detectorchemistryMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationInstrumentationCharged currentParticle Physics - Experiment
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RECENT RESULTS FROM AMANDA

2001

We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope.

PhysicsNuclear and High Energy PhysicsMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrophysicsSolar neutrino problemAtomic and Molecular Physics and OpticsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysics::Atmospheric and Oceanic PhysicsCharged currentInternational Journal of Modern Physics A
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Neutrino energy reconstruction and the shape of the charged current quasielastic-like total cross section

2012

We show that because of the multinucleon mechanism effects, the algorithm used to reconstruct the neutrino energy is not adequate when dealing with quasielastic-like events, and a distortion of the total flux-unfolded cross-section shape is produced. This amounts to a redistribution of strength from high to low energies, which gives rise to a sizable excess (deficit) of low (high) energy neutrinos. This distortion of the shape leads to a good description of the MiniBooNE unfolded charged current quasielastic-like cross sections published by A. A. Aguilar-Arevalo et al. [(MiniBooNE Collaboration), Phys. Rev. D 81, 092005 (2010)]. However, these changes in the shape are artifacts of the unfol…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSolar neutrinoMany-body theoryFísicaSolar neutrino problem01 natural sciencesNuclear physicsMiniBooNE0103 physical sciencesMeasurements of neutrino speedNeutrino010306 general physicsNeutrino oscillationCharged current
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Neutrino observatories can characterize cosmic sources and neutrino properties

2003

Neutrino telescopes that measure relative fluxes of ultrahigh-energy $\nu_{e}, \nu_{\mu}, \nu_{\tau}$ can give information about the location and characteristics of sources, about neutrino mixing, and can test for neutrino instability and for departures from CPT invariance in the neutrino sector. We investigate consequences of neutrino mixing for the neutrino flux arriving at Earth, and consider how terrestrial measurements can characterize distant sources. We contrast mixtures that arise from neutrino oscillations with those signaling neutrino decays. We stress the importance of measuring $\nu_{e}, \nu_{\mu}, \nu_{\tau}$ fluxes in neutrino observatories.

PhysicsNuclear and High Energy PhysicsParticle physicsCOSMIC cancer databaseCPT symmetryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSolar neutrino problemAstrophysicsNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationMixing (physics)Computer Science::Databases
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Lepton physics versus neutrino mass

1990

Abstract The relationship between the strength of lepton flavour violating processes and the magnitude of the neutrino mass is rather model dependent. I review this question within different neutrino mixing models including superstring inspired models. Processes such as μ → e + γ , μ → 3 e , μ - e conversion in nuclei, etc. as well as lepton flavour violating Z ° decays can occur even if the physical neutrinos are strictly massless. As a result, the corresponding rates are unconstrained by bounds on the neutrino mass that follow from laboratory, astrophysics and cosmology and can therefore be large. Leptonic CP violation may also occur even when the physical neutrinos are strictly massless.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologySuperstring theoryAtomic and Molecular Physics and OpticsCosmologyNuclear physicsMassless particleCP violationMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLeptonNuclear Physics B - Proceedings Supplements
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Absolute neutrino mass scale from flavor symmetries

2013

Abstract The 2012 has been an important year for neutrino physics, current data are reviewed and compared with 2011 global fit. Models based on discrete flavor symmetries predict neutrino mass mass sum-rule (MSR), which is useful to reduce the number of independent model parameters. We found that only four classes of MSR are possible. Such neutrino MSRs constrain the absolute neutrino mass scale. We study the implications of these mass relations for the lightest neutrino mass and for the lower bound of the effective mass m e e of the neutrinoless double beta decay.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyUpper and lower boundsAtomic and Molecular Physics and OpticsNuclear physicsEffective mass (solid-state physics)Double beta decayHomogeneous spaceMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationFlavorNuclear Physics B - Proceedings Supplements
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Pulsar Velocities without Neutrino Mass

1998

We show that pulsar velocities may arise from anisotropic neutrino emission induced by resonant conversions of massless neutrinos in the presence of a strong magnetic field. The main ingredient is a small violation of weak universality and neither neutrino masses nor magnetic moments are required.

PhysicsNuclear and High Energy PhysicsParticle physicsMagnetic momentPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)General Physics and AstronomyFísicaFOS: Physical sciencesElementary particleSolar neutrino problemAstrophysicsAtomic and Molecular Physics and OpticsMagnetic fieldMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)PulsarMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLepton
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A large magnetic detector for the neutrino factory

2000

Abstract The physics opportunities of the neutrino factory have been the subject of a number of recent studies. It was shown that sensitive measurements of the angle θ 13 , of MSW effects, and of the sign of the atmospheric mass difference Δ m 23 2 are possible, and even CP violation in the neutrino mixing matrix may be within reach. The focus of interest is the oscillation ν e →ν μ , which leads in the well-defined neutrino beam of the neutrino factory to ‘wrong-sign’ muon events. In this paper, we show that a large magnetic detector will be capable of detecting with high efficiency and small backgrounds such wrong-sign muon events. We present a conceptual design of the apparatus and its p…

PhysicsNuclear and High Energy PhysicsParticle physicsMuonPhysics::Instrumentation and DetectorsPontecorvo–Maki–Nakagawa–Sakata matrixSolar neutrino problemNuclear physicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino FactoryNeutrinoNeutrino oscillationInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Neutrino mixing and future accelerator neutrino experiments

1992

PhysicsNuclear and High Energy PhysicsParticle physicsNeutrino detectorSolar neutrinoMeasurements of neutrino speedNeutrinoSolar neutrino problemNeutrino oscillationAtomic and Molecular Physics and OpticsMixing (physics)Nuclear Physics B - Proceedings Supplements
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