Search results for "Oscillation"

showing 10 items of 1257 documents

Mass Varying Neutrinos in the Sun

2005

In this work we study the phenomenological consequences of the dependence of mass varying neutrinos on the neutrino density in the Sun, which we precisely compute in each point along the neutrino trajectory. We find that a generic characteristic of these scenarios is that they establish a connection between the effective Delta m^2 in the Sun and the absolute neutrino mass scale. This does not lead to any new allowed region in the oscillation parameter space. On the contrary, due to this effect, the description of solar neutrino data worsens for large absolute mass. As a consequence a lower bound on the level of degeneracy can be derived from the combined analysis of the solar and KamLAND da…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesParameter spaceAstrophysics01 natural sciences7. Clean energyUpper and lower boundsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsStandard solar model010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaSolar neutrino problemHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Status of global fits to neutrino oscillations

2004

We review the present status of global analyses of neutrino oscillations, taking into account the most recent neutrino data including the latest KamLAND and K2K updates presented at Neutrino2004, as well as state-of-the-art solar and atmospheric neutrino flux calculations. We give the two-neutrino solar + KamLAND results, as well as two-neutrino atmospheric + K2K oscillation regions, discussing in each case the robustness of the oscillation interpretation against departures from the Standard Solar Model and the possible existence of non-standard neutrino physics. Furthermore, we give the best fit values and allowed ranges of the three-flavour oscillation parameters from the current worlds' …

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsStandard solar modelDegree (graph theory)010308 nuclear & particles physicsOscillationAnomaly (natural sciences)Astrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSolar neutrino problemAtomic and Molecular Physics and Opticsddc:High Energy Physics - Phenomenology13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrino
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Updating neutrino magnetic moment constraints

2016

20 pages.- 4 figures.- Addendum on the limit from the Borexino data

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelFOS: Physical sciencesElectromagnetic properties01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationMajorana neutrinosBorexinoPhysicsMagnetic moment010308 nuclear & particles physicslcsh:QC1-999High Energy Physics - PhenomenologyNucleus coherent scatteringMeasurements of neutrino speedCP violationBorexinoNeutrinolcsh:Physics
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Search for short baseline nu(e) disappearance with the T2K near detector

2015

8 pages.- 6 figures

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoAstronomy & AstrophysicsNeutrino beam7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillation0206 Quantum PhysicsNeutrino fluxPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsPhysicsDetectorT2K experimentNuclear & Particles Physics0201 Astronomical And Space SciencesPhysical Sciences
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Status of Light Sterile Neutrino Searches

2020

A number of anomalous results in short-baseline oscillation may hint at the existence of one or more light sterile neutrino states in the eV mass range and have triggered a wave of new experimental efforts to search for a definite signature of oscillations between active and sterile neutrino states. The present paper aims to provide a comprehensive review on the status of light sterile neutrino searches in mid-2019: we discuss not only the basic experimental approaches and sensitivities of reactor, source, atmospheric, and accelerator neutrino oscillation experiments but also the complementary bounds arising from direct neutrino mass experiments and cosmological observations. Moreover, we r…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBibliographyddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsOscillationHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Cosmological modelHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Dirac neutrinos from flavor symmetry

2013

We present a model where Majorana neutrino mass terms are forbidden by the flavor symmetry group Delta(27). Neutrinos are Dirac fermions and their masses arise in the same way as that of the charged fermions, due to very small Yukawa couplings. The model fits current neutrino oscillation data and correlates the octant of the atmospheric angle with the magnitude of the lightest neutrino mass, with maximal mixing excluded for any neutrino mass

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoNeutrino theory of lightPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::LatticePontecorvo–Maki–Nakagawa–Sakata matrixFOS: Physical sciences7. Clean energy01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyDirac fermionsymbolsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Limits on sterile neutrino contributions to neutrinoless double beta decay

2015

Nuclear matrix elements (NME) for exchange of arbitrary mass neutrinos are calculated in the interacting boson model (IBM-2). By combining the NME with the phase space factors (PSF), expected half-lives for neutrinos of mass ${m}_{N}$ and coupling ${U}_{eN}$ are estimated. Limits on sterile neutrinos with masses in the eV, keV, MeV-GeV, and TeV range are given.

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesdouble beta decaynuclear matrix elements7. Clean energydark matterNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)sterile neutrinosDouble beta decayNuclear ExperimentNeutrino oscillationPhysicsta114High Energy Physics::PhenomenologySolar neutrino problemCoupling (probability)High Energy Physics - PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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The T2K Experiment

2011

The T2K experiment is a long-baseline neutrino oscillation experiment. Its main goal is to measure the last unknown lepton sector mixing angle {\theta}_{13} by observing {\nu}_e appearance in a {\nu}_{\mu} beam. It also aims to make a precision measurement of the known oscillation parameters, {\Delta}m^{2}_{23} and sin^{2} 2{\theta}_{23}, via {\nu}_{\mu} disappearance studies. Other goals of the experiment include various neutrino cross section measurements and sterile neutrino searches. The experiment uses an intense proton beam generated by the J-PARC accelerator in Tokai, Japan, and is composed of a neutrino beamline, a near detector complex (ND280), and a far detector (Super-Kamiokande)…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and Detectorsddc:500.27. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Long baseline[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinos010306 general physicsNeutrino oscillationphysics.ins-detInstrumentationQCPhysicsT2Khep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyT2K experimentNeutrinos; Neutrino oscillation; Long baseline; T2K; J-PARC; Super-KamiokandeFísicaNeutrino detectorJ-PARCHigh Energy Physics::ExperimentJ-PARCSuper-KamiokandeNeutrinoSuper-KamiokandeLepton
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Constraining the invisible neutrino decay with KM3NeT-ORCA

2019

Several theories of particle physics beyond the Standard Model consider that neutrinos can decay. In this work we assume that the standard mechanism of neutrino oscillations is altered by the decay of the heaviest neutrino mass state into a sterile neutrino and, depending on the model, a scalar or a Majoron. We study the sensitivity of the forthcoming KM3NeT-ORCA experiment to this scenario and find that it could improve the current bounds coming from oscillation experiments, where three-neutrino oscillations have been considered, by roughly two orders of magnitude. We also study how the presence of this neutrino decay can affect the determination of the atmospheric oscillation parameters $…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaNeutrino masses and mixingScalar (mathematics)FOS: Physical sciences01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationNeutrino decayMajoronPhysics010308 nuclear & particles physicsOscillationNeutrino oscillationsHigh Energy Physics::Phenomenologylcsh:QC1-999High Energy Physics - PhenomenologyKM3NeTHigh Energy Physics::ExperimentNeutrinoNeutrino telescopeslcsh:PhysicsPhysics Letters
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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