Search results for "Measurement"

showing 10 items of 2918 documents

Dilepton photoproduction on a deuteron target

2019

We investigate the sensitivity of the cross section for lepton pair production off a deuteron target, $\gamma d \to l^+ l^- d$, to the deuteron charge radius. We show that for small momentum transfers the Bethe-Heitler process dominates, and that it is sensitive to the charge radius such that a cross section ratio measurement of about $0.1 \%$ relative accuracy could give a deuteron charge radius more accurate that the current electron scattering value and sufficiently accurate to distinguish between the electronic and muonic atomic values.

PhysicsNuclear and High Energy PhysicsNuclear Theory010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciences01 natural sciences7. Clean energylcsh:QC1-999Nuclear physicsMomentumNuclear Theory (nucl-th)Cross section (physics)High Energy Physics - PhenomenologyPair productionHigh Energy Physics - Phenomenology (hep-ph)DeuteriumCharge radius0103 physical sciencesRatio measurement010306 general physicsElectron scatteringlcsh:PhysicsLepton
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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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Precision measurement of the mass of the tau lepton

2014

An energy scan near the $\tau$ pair production threshold has been performed using the BESIII detector. About $24$ pb$^{-1}$ of data, distributed over four scan points, was collected. This analysis is based on $\tau$ pair decays to $ee$, $e\mu$, $eh$, $\mu\mu$, $\mu h$, $hh$, $e\rho$, $\mu\rho$ and $\pi\rho$ final states, where $h$ denotes a charged $\pi$ or $K$. The mass of the $\tau$ lepton is measured from a maximum likelihood fit to the $\tau$ pair production cross section data to be $m_{\tau} = (1776.91\pm0.12 ^{+0.10}_{-0.13}$) MeV/$c^2$, which is currently the most precise value in a single measurement.

PhysicsNuclear and High Energy PhysicsParticle physicsAnnihilation010308 nuclear & particles physicshep-exElectron–positron annihilationMaximum likelihoodSingle measurementDetectorBESIII01 natural sciencesDECAYSHigh Energy Physics - ExperimentNuclear physicsENERGYPair production0103 physical sciencesRADIATIVE-CORRECTIONSHigh Energy Physics::Experiment010306 general physicsANNIHILATIONDETECTORSYSTEMLepton
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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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Relic Neutrino Decoupling Including Flavour Oscillations

2005

In the early universe, neutrinos are slightly coupled when electron-positron pairs annihilate transferring their entropy to photons. This process originates non-thermal distortions on the neutrino spectra which depend on neutrino flavour, larger for nu_e than for nu_mu or nu_tau. We study the effect of three-neutrino flavour oscillations on the process of neutrino decoupling by solving the momentum-dependent kinetic equations for the neutrino spectra. We find that oscillations do not essentially modify the total change in the neutrino energy density, giving N_eff=3.046 in terms of the effective number of neutrinos, while the small effect over the production of primordial 4He is increased by…

PhysicsNuclear and High Energy PhysicsParticle physicsPhotonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFlavourAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaNeutrino decouplingSolar neutrino problemAstrophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLepton
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