Search results for "Oscillation"

showing 10 items of 1257 documents

Robust signatures of solar neutrino oscillation solutions

2001

With the goal of identifying signatures that select specific neutrino oscillation parameters, we test the robustness of global oscillation solutions that fit all the available solar and reactor experimental data. We use three global analysis strategies previously applied by different authors and also determine the sensitivity of the oscillation solutions to the critical nuclear fusion cross section, S_{17}(0), for the production of 8B. The favored solutions are LMA, LOW, and VAC in order of g.o.f. The neutral current to charged current ratio for SNO is predicted to be 3.5 +- 0.6 (1 sigma), which is separated from the no-oscillation value of 1.0 by much more than the expected experimental er…

Nuclear and High Energy PhysicsParticle physicsNuclear TheorySolar neutrinoFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentStandard ModelNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentBorexinoCharged currentParticle Physics - PhenomenologyPhysicsStandard solar model010308 nuclear & particles physicsOscillationAstrophysics (astro-ph)FísicaHigh Energy Physics - Phenomenology13. Climate actionHigh Energy Physics::ExperimentNeutrino
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Photon emission in neutral-current interactions at intermediate energies

2013

Neutral current photon emission reactions with nucleons and nuclei are studied. These processes are important backgrounds for nu_mu to nu_e (bar(nu)_mu to bar(nu)_e) appearance oscillation experiments where electromagnetic showers instigated by electrons (positrons) and photons are not distinguishable. At intermediate energies, these reactions are dominated by the weak excitation of the Delta(1232) resonance and its subsequent decay into Ngamma There are also non-resonant contributions that, close to threshold, are fully determined by the effective chiral Lagrangian of strong interactions. In addition, we have also included mechanisms mediated by nucleon excitations (N*) from the second res…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryStrong interactionNuclear TheoryFOS: Physical sciencesElectron01 natural sciencesResonance (particle physics)High Energy Physics - ExperimentNuclear Theory (nucl-th)symbols.namesakeHigh Energy Physics - Experiment (hep-ex)Pauli exclusion principleHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsNeutral current010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - Phenomenology13. Climate actionsymbolsHigh Energy Physics::ExperimentNeutrinoAtomic physicsNucleon
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Atmospheric neutrino oscillations and new physics

2004

We study the robustness of the determination of the neutrino masses and mixing from the analysis of atmospheric and K2K data under the presence of different forms of phenomenologically allowed new physics in the nu_mu--nu_tau sector. We focus on vector and tensor-like new physics interactions which allow us to treat, in a model independent way, effects due to the violation of the equivalence principle, violations of the Lorentz invariance both CPT conserving and CPT violating, non-universal couplings to a torsion field and non-standard neutrino interactions with matter. We perform a global analysis of the full atmospheric data from SKI together with long baseline K2K data in the presence of…

Nuclear and High Energy PhysicsParticle physicsOscillationsPhysics beyond the Standard ModelFOS: Physical sciencesLorentz covariance01 natural sciencesTorsion fieldPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)Robustness (computer science)0103 physical sciencesOscil·lacionsNeutrinsNeutrinos010306 general physicsNeutrino oscillationMixing (physics)Particles (Nuclear physics)PhysicsViolació càrrega-paritat (Física nuclear)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoAtmospheric neutrinoCP violation (Nuclear physics)Physical Review D
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Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II

2009

The AMANDA-II detector, operating since 2000 in the deep ice at the geographic South Pole, has accumulated a large sample of atmospheric muon neutrinos in the 100 GeV to 10 TeV energy range. The zenith angle and energy distribution of these events can be used to search for various phenomenological signatures of quantum gravity in the neutrino sector, such as violation of Lorentz invariance (VLI) or quantum decoherence (QD). Analyzing a set of 5511 candidate neutrino events collected during 1387 days of livetime from 2000 to 2006, we find no evidence for such effects and set upper limits on VLI and QD parameters using a maximum likelihood method. Given the absence of evidence for new flavor-…

Nuclear and High Energy PhysicsParticle physicsOscillationsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaConfidence-IntervalsGravityFOS: Physical sciencesGeneratorLorentz covariance01 natural sciences7. Clean energyHigh Energy Physics - ExperimentScatteringHigh Energy Physics - Experiment (hep-ex)SensitivityQuantum Decoherence0103 physical sciencesddc:530Muon neutrino010306 general physicsNeutrino oscillationTelescopeAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSmall SignalsLorentz Invariance Violation
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Gravitino dark matter and neutrino masses with bilinear R-parity violation

2011

Bilinear R-parity violation provides an attractive origin for neutrino masses and mixings. In such schemes the gravitino is a viable decaying dark matter particle whose R-parity violating decays lead to monochromatic photons with rates accessible to astrophysical observations. We determine the parameter region allowed by gamma-ray line searches, dark matter relic abundance and neutrino oscillation data, obtaining a limit on the gravitino mass $m_{\tilde G} \lsim$ 1-10 GeV corresponding to a relatively low reheat temperature $T_R \lsim$ few $\times 10^7-10^8$ GeV. Neutrino mass and mixing parameters may be reconstructed at accelerator experiments like the Large Hadron Collider.

Nuclear and High Energy PhysicsParticle physicsPhotonAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesMasas de neutrinos01 natural sciencesNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)R-paridad bilinealR-parity0103 physical sciences010306 general physicsNeutrino oscillationLine (formation)PhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyGravitinoHigh Energy Physics::ExperimentNeutrinoGravitino
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Resolving the octant of theta(23) with T2K and NOvA

2013

Preliminary results of MINOS experiment indicate that theta(23) is not maximal. Global fits to world neutrino data suggest two nearly degenerate solutions for theta(23): one in the lower octant (LO: theta(23) 45 degrees). v(mu) -> v(e) oscillations in superbeam experiments are sensitive to the octant and are capable of resolving this degeneracy. We study the prospects of this resolution by the current T2K and upcoming NOvA experiments. Because of the hierarchy-delta(CP) degeneracy and the octant delta(CP) degeneracy, the impact of hierarchy on octant resolution has to be taken into account. As in the case of hierarchy determination, there exist favorable (unfavorable) values of delta(CP) fo…

Nuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsFOS: Physical sciencesSilver ChannelOctant (solid geometry)01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Oscillation ExperimentsNeutrino Physics010306 general physicsNeutrino oscillationPhysicsNOνAMixing Matrix010308 nuclear & particles physicsDegenerate energy levelsCp ViolationInstrumentation and Detectors (physics.ins-det)High Energy Physics - PhenomenologyCP violationMINOSBeyond Standard ModelLine-Experiment-SimulatorMass MatrixCP violationNeutrinoIndraStra Global
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Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data

2014

We present a measurement of neutrino oscillations via atmospheric muon neutrino disappearance with three years of data of the completed IceCube neutrino detector. DeepCore, a region of denser instrumentation, enables the detection and reconstruction of atmospheric muon neutrinos between 10 GeV and 100 GeV, where a strong disappearance signal is expected. The detector volume surrounding DeepCore is used as a veto region to suppress the atmospheric muon background. Neutrino events are selected where the detected Cherenkov photons of the secondary particles minimally scatter, and the neutrino energy and arrival direction are reconstructed. Both variables are used to obtain the neutrino oscilla…

Nuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsTELESCOPEPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)TRACK RECONSTRUCTIONMuon neutrinoddc:530Neutrino oscillationPhysicsHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Solar neutrino problemPERFORMANCENeutrino detectorPhysics and AstronomyMeasurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoNeutrino astronomySYSTEM
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Prediction of neutrino fluxes in the NOMAD experiment

2003

The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD are predicted with an uncertainty of about 8% for nu(mu) and nu(e), 10% for antinu(mu), and…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationInstrumentationCharged currentPhysicsNeutral current010308 nuclear & particles physicsDetectorHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemMagnetic fieldBeamlineHigh Energy Physics::ExperimentNeutrinoParticle Physics - Experiment
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Global constraints on muon-neutrino non-standard interactions

2011

The search for new interactions of neutrinos beyond those of the Standard Model may help to elucidate the mechanism responsible for neutrino masses. Here we combine existing accelerator neutrino data with restrictions coming from a recent atmospheric neutrino data analysis in order to lift parameter degeneracies and improve limits on new interactions of muon neutrinos with quarks. In particular we re-consider the results of the NuTeV experiment in view of a new evaluation of its systematic uncertainties. We find that, although constraints for muon neutrinos are better than those applicable to tau or electron neutrinos, they lie at the few $\times 10^{-2}$ level, not as strong as previously …

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGrand Unified TheoryMuon neutrinoFermilabNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoLepton
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Probing neutralino properties in minimal supergravity with bilinear R-parity violation

2012

Supersymmetric models with bilinear R-parity violation (BRPV) can account for the observed neutrino masses and mixing parameters indicated by neutrino oscillation data. We consider minimal supergravity versions of BRPV where the lightest supersymmetric particle (LSP) is a neutralino. This is unstable, with a large enough decay length to be detected at the CERN Large Hadron Collider (LHC). We analyse the LHC potential to determine the LSP properties, such as mass, lifetime and branching ratios, and discuss their relation to neutrino properties.

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsBilinear interpolationFOS: Physical sciencesSupergravity01 natural sciences7. Clean energyLightest Supersymmetric ParticleSupergravitaciónHigh Energy Physics - Phenomenology (hep-ph)R-parity0103 physical sciencesNeutrinos010306 general physicsNeutrino oscillationPhysicsNeutrinesLarge Hadron Collider010308 nuclear & particles physicsSupergravityHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyNeutralinoHigh Energy Physics::ExperimentNeutrino
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