Search results for "sterile"

showing 10 items of 164 documents

The Seesaw Scale vs Cosmology

2015

We will study the simplest extension of the Standard Model that can account for neutrino masses: the Type-I seesaw. The model introduces a New Physics scale, M, which is often assumed to be much larger than the electroweak scale. However, it is presently unconstrained and the light neutrino masses and mixing can be generated for any value of M above O(eV). Paying special attention to the contribution of the sterile states to Neff as a function of M, we will show that a large part of the M parameter space (8 orders of magnitude) can be excluded thanks to cosmological measurements. The implications for neutrinoless double beta decay will be discussed too.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologySolar neutrino problemSeesaw molecular geometryMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoElectroweak scaleNeutrino oscillationComputer Science::DatabasesNuclear and Particle Physics Proceedings
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Neutrino Masses and Mixing one Decade from Now

2000

We review the status of neutrino masses and mixings in the light of the solar and atmospheric neutrino data. The result from the LSND experiment is also considered. We discuss the present knowledge and the expected sensitivity to the neutrino mixing parameters in the simplest schemes proposed to reconcile these data some of which include a light sterile neutrino in addition to the three standard ones.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentSensitivity (control systems)NeutrinoAtmospheric neutrinoInstrumentationMixing (physics)
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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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Nucleosynthesis constraints on active-sterile neutrino conversions in the early universe with random magnetic field

1994

We consider active-sterile neutrino conversions in the early universe hot plasma in the presence of a random magnetic field generated at the electroweak phase transition. Within a random field domain the magnetization asymmetry of the lepton antilepton plasma produced by a uniform constant magnetic field is huge in contrast to their small density asymmetry, leading to a drastic change in the active-sterile conversion rates. Assuming that the random field provides the seed for the galactic field one can estimate the restrictions from primordial nucleosynthesis. Requiring that the extra sterile \neu does not enter in equilibrium with the active ones before nucleosynthesis we find limits of th…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsRandom fieldField (physics)media_common.quotation_subjectHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisNucleosynthesisHigh Energy Physics::ExperimentNeutrinomedia_commonLeptonNuclear Physics B
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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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