Search results for " oscillation"

showing 10 items of 845 documents

Quantum decoherence and neutrino data

2006

In this work we perform global fits of microscopic decoherence models of neutrinos to all available current data, including LSND and KamLAND spectral distortion results. In previous works on related issues the models used were supposed to explain LSND results by means of quantum gravity induced decoherence. However those models were purely phenomenological without any underlying microscopic basis. It is one of the main purposes of this article to use detailed microscopic decoherence models with complete positivity, to fit the data.The decoherence in these models has contributions not only from stochastic quantum gravity vacua operating as a medium, but also from conventional uncertainties i…

PhysicsNuclear and High Energy PhysicsQuantum decoherenceOscillationFOS: Physical sciencesFísicaNeutrino beamHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanicsQuantum gravityHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationOrder of magnitudeEnergy (signal processing)Nuclear Physics B
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Recent Developments in Neutrino/Antineutrino-Nucleus Interactions

2012

Recent experimental results and developments in the theoretical treatment of neutrino-nucleus interactions in the energy range of 1–10 GeV are discussed. Difficulties in extracting neutrino-nucleon cross sections from neutrino-nucleus scattering data are explained and significance of understanding nuclear effects for neutrino oscillation experiments is stressed. Detailed discussions of the status of two-body current contribution in the kinematic region dominated by quasielastic scattering and specific features of partonic nuclear effects in weak DIS scattering are presented.

PhysicsNuclear and High Energy PhysicsQuasielastic scatteringParticle physicsNeutral current010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyNuclear TheoryFísicaDeep inelastic scattering01 natural scienceslcsh:QC1-999Nuclear physics0103 physical sciencesBibliographyHigh Energy Physics::ExperimentNeutrinoNuclear Experiment010306 general physicsNeutrino oscillationlcsh:PhysicsCharged currentAdvances in High Energy Physics
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Performance of long modules of silicon microstrip detectors

1998

This note describes the performance of modules assembled with up to twelve silicon microstrip detectors. These modules were built for the instrumented Silicon Target (STAR) that has been installed in the NOMAD spectrometer. Laboratory and test beam results are compared with model predictions. For a module of nine detectors, test beam results indicate a signal--to--noise ratio of 19, a hit finding efficiency of 99.8\% and a spatial resolution of 6.0 $\mu$m. Laboratory measurements indicate that modules of twelve detectors exhibit a signal--to--noise ratio of the order of 16.

PhysicsNuclear and High Energy PhysicsSpectrometerSiliconbusiness.industryPhysics::Instrumentation and DetectorsDetectorchemistry.chemical_elementFísicaParticle detectorSemiconductor detectorNuclear physicssilicon microstrip detectors; neutrino oscillationsSignal-to-noise ratioOpticschemistryMeasuring instrumentHigh Energy Physics::ExperimentDetectors and Experimental TechniquesbusinessInstrumentationImage resolution
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Oscillations of Dirac and Majorana neutrinos in matter and a magnetic field

2008

We study the evolution of massive mixed Dirac and Majorana neutrinos in matter under the influence of a transversal magnetic field. The analysis is based on relativistic quantum mechanics. We solve exactly the evolution equation for relativistic neutrinos, find the neutrino wave functions, and calculate the transition probability for spin-flavor oscillations. We analyze the dependence of the transition probability on the external fields and compare the cases of Dirac and Majorana neutrinos. The evolution of Majorana particles in vacuum is also studied and correction terms to the standard oscillation formula are derived and discussed. As a possible application of our results we discuss the s…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDirac (software)FOS: Physical sciencesRelativistic quantum mechanics01 natural sciencesHigh Energy Physics - PhenomenologyMAJORANAsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Dirac fermionQuantum electrodynamics0103 physical sciencessymbolsHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationMajorana equationPhysical Review D
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Minimal models with light sterile neutrinos

2011

We study the constraints imposed by neutrino oscillation experiments on the minimal extensions of the Standard Model (SM) with $n_R$ gauge singlet fermions ("right-handed neutrinos"), that can account for neutrino masses. We consider the most general coupling to SM fields of the new fields, in particular those that break lepton number and we do not assume any a priori hierarchy in the mass parameters. We proceed to analyze these models starting from the lowest level of complexity, defined by the number of extra fermionic degrees of freedom. The simplest choice that has enough free parameters in principle (i.e. two mass differences and two angles) to explain the confirmed solar and atmospher…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsFOS: Physical sciencesFísica01 natural sciences7. Clean energyLepton numberStandard ModelMiniBooNEHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry13. Climate action0103 physical sciencesNeutrino010306 general physicsNeutrino oscillation
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Low-scale seesaw models versusNeff

2014

We consider the contribution of the extra sterile states in generic low-scale seesaw models to extra radiation, parametrized by ${N}_{\text{eff}}$. We find that the value of ${N}_{\text{eff}}$ is roughly independent of the seesaw scale within a wide range. We explore the full parameter space in the case of two extra sterile states and find that these models are strongly constrained by cosmological data for any value of the seesaw scale below $\mathcal{O}(100\text{ }\text{ }\mathrm{MeV})$.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFísicaScale (descriptive set theory)Parameter space01 natural sciencesSeesaw molecular geometry0103 physical sciences010306 general physicsNeutrino oscillationPhysical Review D
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The Minimal 3 + 2 Neutrino Model vs. Higgs Decays

2016

Abstract The minimal 3+2 neutrino model is a Type-I seesaw model with two Weyl fermions, singlets under the Standard Model. Apart from light neutrino masses and mixings, this model can be fully described by four additional parameters. In this work, we study the minimal 3+2 neutrino model in scenarios where the singlets have masses at the GeV scale. This can lead to Higgs decays into heavy neutrinos, which could be observable as displaced vertices at the LHC.

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFermion01 natural sciencesStandard ModelSeesaw molecular geometry0103 physical sciencesHiggs bosonMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationNuclear and Particle Physics Proceedings
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Constraints on massive sterile neutrino species from current and future cosmological data

2011

Sterile massive neutrinos are a natural extension of the Standard Model of elementary particles. The energy density of the extra sterile massive states affects cosmological measurements in an analogous way to that of active neutrino species. We perform here an analysis of current cosmological data and derive bounds on the masses of the active and the sterile neutrino states as well as on the number of sterile states. The so-called (3+2) models with three sub-eV active massive neutrinos plus two sub-eV massive sterile species is well within the 95% CL allowed regions when considering cosmological data only. If the two extra sterile states have thermal abundances at decoupling, Big Bang Nucle…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::PhenomenologyCosmic background radiationFOS: Physical sciencesFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsDecoupling (cosmology)CosmologyHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesissymbolsQuantitative Biology::Populations and EvolutionHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawPhysical Review D
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Neutrino Masses, Grand Unification, and Baryon Number Violation

2014

If grand unification is real, searches for baryon-number violation should be included on the list of observables that may reveal information regarding the origin of neutrino masses. Making use of an effective-operator approach and assuming that nature is SU(5) invariant at very short distances, we estimate the consequences of different scenarios that lead to light Majorana neutrinos for low-energy phenomena that violate baryon number minus lepton number (B-L) by two (or more) units, including neutron-antineutron oscillations and B-L violating nucleon decays. We find that, among all possible effective theories of lepton-number violation that lead to nonzero neutrino masses, only a subset is,…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesLepton numberHigh Energy Physics - PhenomenologyMAJORANAGrand unification epochHigh Energy Physics - Phenomenology (hep-ph)Grand Unified TheoryHigh Energy Physics::ExperimentBaryon numberNeutrinoNeutrino oscillation
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Non-standard interactions with high-energy atmospheric neutrinos at IceCube

2017

Non-standard interactions in the propagation of neutrinos in matter can lead to significant deviations from expectations within the standard neutrino oscillation framework and atmospheric neutrino detectors have been considered to set constraints. However, most previous works have focused on relatively low-energy atmospheric neutrino data. Here, we consider the one-year high-energy through-going muon data in IceCube, which has been already used to search for light sterile neutrinos, to constrain new interactions in the $\mu\tau$-sector. In our analysis we include several systematic uncertainties on both, the atmospheric neutrino flux and on the detector properties, which are accounted for v…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physicsMuon010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyHadronFOS: Physical sciencesFlux7. Clean energy01 natural sciencesSpectral line3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)13. Climate action0103 physical sciencesHigh Energy Physics::ExperimentSensitivity (control systems)Neutrino010306 general physicsNeutrino oscillationJournal of High Energy Physics
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