Search results for "oscillation"

showing 10 items of 1257 documents

Neutrino masses, leptogenesis, and dark matter in a hybrid seesaw model

2009

4 pages.-- ISI article identifier:000263816600020.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0811.0953

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFísicaStandard ModelNuclear physicsSeesaw mechanismSeesaw molecular geometryLeptogenesisHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Physics at new accelerators: Looking beyond the Standard Model

1993

Abstract Neutrino masses can have important implications in nuclear and particle physics, astrophysics and cosmology. Apart from the effects related to solar neutrinos, neutrino oscillations, dark matter, beta and double beta decays, massive neutrinos can also produce signals in the new accelerators. Here I focus on μ and τ number violating processes, very promising for muon and tau factories, as well as on the signatures associated with spontaneously broken R parity supersymmetry and neutral heavy leptons. These include the possibility of high rates for single chargino and neutralino production at LEP, LHC/SSC, as well as new signatures involving invisibly decaying Higgs bosons.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelSolar neutrinoHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemAtomic and Molecular Physics and OpticsNuclear physicsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLeptonParticle Physics - Phenomenology
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Neutrino magnetic moments and low-energy solar neutrino-electron scattering experiments

1998

The scattering of solar neutrinos on electrons is sensitive to the neutrino magnetic moments through an interference of electromagnetic and weak amplitudes in the cross section. We show that future low-energy solar neutrino experiments with good angular resolution can be sensitive to the resulting azimuthal asymmetries in event number and should provide useful information on non-standard neutrino properties such as magnetic moments. We compare asymmetries expected at HELLAZ (mainly pp neutrinos) with those at the Kamiokande and Super-Kamiokande experiments (Boron neutrinos), both for the case of Dirac and Majorana neutrinos and discuss the advantages of low energies. Potentially interesting…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)FísicaFOS: Physical sciencesSolar neutrino problemAstrophysicsNuclear physicsCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Reconciling neutrino anomalies in a simple four-neutrino scheme with R-parity violation

2000

We propose a simple extension of the MSSM based on extra compact dimensions which includes an $SU(2) \otimes U(1)$ singlet superfield. The fermion present in this superfield is the sterile neutrino, which combines with one linear combination of $\nu_e-\nu_{\mu}-\nu_{\tau}$ to form a Dirac pair whose mass accounts for the LSND anomaly. Its small mass can be ascribed to a volume suppression factor associated with extra compact dimensions. On the other hand the sterile neutrino scalar partner can trigger the spontaneous violation of R-parity, thereby inducing the necessary mass splittings to fit also the solar and atmospheric neutrino data. Thus the model can explain all neutrino oscillation d…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaFermionLepton numberLightest Supersymmetric ParticleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)R-parityHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Effects of sterile neutrinos on the ultrahigh-energy cosmic neutrino flux

2003

We investigate the effect of sterile neutrinos that are nearly degenerate with active ones on the flux of ultrahigh-energy cosmic ray neutrinos at earth. This offers a way to probe neutrino oscillations in the mass-squared range (10^{-16} eV^2 < ��m^2 < 10^{-11} eV^2) which maybe hard to detect by any other means. Taking into account the present experimental uncertainties of the active-active mixing angles and by allowing any values for the active-sterile mixing angles we find that the ratio of the electron and muon neutrino fluxes may change by -40 % to 70 % in comparison with the ratio in the absence of active-sterile mixing.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Status of the MSW Solutions to the Solar Neutrino Problem

2000

In this talk we present the results of an updated global analysis of two-flavor MSW solutions to the solar neutrino problem in terms of conversions of $\nu_e$ into active or sterile neutrinos including the the full data set corresponding to the 825-day Super-Kamiokande data sample as well as to Chlorine, GALLEX and SAGE experiments.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsSolar neutrinoSAGEHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Full dataHigh Energy Physics::ExperimentGALLEXNeutrino oscillation
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On the description of non-unitary neutrino mixing

2015

28 pages.- 8 figures.- typos corrected.- modified bounds on non-unitarity parameters.- new figs 3 and 4

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsUnitarityPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixFísicaFOS: Physical sciencesDouble beta decayHigh Energy Physics - ExperimentStandard Model (mathematical formulation)High Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Heavy majorana neutrinosMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Constraining neutrino oscillation parameters with current solar and atmospheric data

2002

We analyze the impact of recent solar, atmospheric and reactor data in the determination of the neutrino oscillation parameters, taking into account that both the solar nu_e and the atmospheric nu_mu may convert to a mixture of active and sterile neutrinos. We use the most recent global solar neutrino data, including the 1496-day Super-K neutrino data sample, and we investigate in detail the impact of the SNO neutral current, spectral and day/night data by performing also an analysis using only the charged current rate from SNO. The implications of the first 145.1 days of KamLAND data on the determination of the solar neutrino parameters are also discussed in detail. We confirm the clear pr…

PhysicsNuclear and High Energy PhysicsSterile neutrinoSudbury Neutrino ObservatoryParticle physicsNeutral currentSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoNeutrino oscillationCharged current
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Status of three-neutrino oscillations after the SNO-salt data

2003

We perform a global analysis of neutrino oscillation data in the framework of three neutrinos, including the recent improved measurement of the neutral current events at SNO. In addition to all current solar neutrino data we take into account the reactor neutrino data from KamLAND and CHOOZ, the atmospheric neutrino data from Super-Kamiokande and MACRO, as well as the first spectral data from the K2K long baseline accelerator experiment. The up-to-date best fit values and allowed ranges of the three-flavour oscillation parameters are determined from these data. Furthermore, we discuss in detail the status of the small parameters alpha = Delta_m^2_Sol / Delta_m^2_Atm and sin^2(theta_13), whi…

PhysicsNuclear and High Energy PhysicsSudbury Neutrino ObservatoryParticle physicsNeutral currentOscillationPhysics::Instrumentation and DetectorsSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaCHOOZNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)CP violationHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Supernova Bounds on Majoron-emitting decays of light neutrinos

2000

Neutrino masses arising from the spontaneous violation of ungauged lepton-number are accompanied by a physical Goldstone boson, generically called Majoron. In the high-density supernova medium the effects of Majoron-emitting neutrino decays are important even if they are suppressed in vacuo by small neutrino masses and/or small off-diagonal couplings. We reconsider the influence of these decays on the neutrino signal of supernovae in the light of recent Super-Kamiokande data on solar and atmospheric neutrinos. We find that majoron-neutrino coupling constants in the range $3\times 10^{-7}\lsim g\lsim 2\times 10^{-5}$ or $g \gsim 3 \times 10^{-4}$ are excluded by the observation of SN1987A. T…

PhysicsNuclear and High Energy PhysicsSudbury Neutrino ObservatoryParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationParticle Physics - PhenomenologyMajoron
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