Search results for "Oscillation"

showing 10 items of 1257 documents

Impact of CP-violation on neutrino lepton number asymmetries revisited

2017

We revisit the effect of the (Dirac) CP-violating phase on neutrino lepton number asymmetries in both mass- and flavor-basis. We found that, even if there are sizable effects on muon- and tau-neutrino asymmetries, the effect on the asymmetry of electron-neutrinos is at most similar to the upper bound set by BBN for initial neutrino degeneracy parameters smaller than order unity. We also found that, for the asymmetries in mass-basis, the changes caused by CP-violation is of sub-\% level which is unlikely to be accesible neither in the current nor in the forthcoming experiments.

Particle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectFOS: Physical sciences01 natural sciencesAsymmetryNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationmedia_commonPhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999Massless particleHigh Energy Physics - PhenomenologyCP violationHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Test of Lorentz and CPT violation with short baseline neutrino oscillation excesses

2011

The sidereal time dependence of MiniBooNE ν[subscript e] and ν[over-bar][subscript e] appearance data is analyzed to search for evidence of Lorentz and CPT violation. An unbinned Kolmogorov–Smirnov (K–S) test shows both the ν[subscript e] and ν[over-bar][subscript e] appearance data are compatible with the null sidereal variation hypothesis to more than 5%. Using an unbinned likelihood fit with a Lorentz-violating oscillation model derived from the Standard Model Extension (SME) to describe any excess events over background, we find that the ν[subscript e] appearance data prefer a sidereal time-independent solution, and the ν[over-bar][subscript e] appearance data slightly prefer a sidereal…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and DetectorsLorentz transformationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMiniBooNEPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsMiniBooNEsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Violació CP (Física nuclear)Standard-Model ExtensionStatistical analysisNeutrino oscillationPhysicsOscillationNull (mathematics)High Energy Physics::PhenomenologyLorentz violationHigh Energy Physics - PhenomenologySidereal timesymbolsHigh Energy Physics::ExperimentPhysics Letters B
researchProduct

Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

2012

We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence l…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectSolar neutrino01 natural sciencesAsymmetrySolar neutrinoNuclear physicsDay-night effect0103 physical sciences010306 general physicsNeutrino oscillationNuclear Experimentday–night effectBorexinomedia_commonPhysicsneutrino oscillations010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemNeutrino detectorsolar neutrinosMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoCPT violation
researchProduct

Single photon events from neutral current interactions at MiniBooNE

2014

The MiniBooNE experiment has reported results from the analysis of $\nu _e$ and $\bar \nu _e$ appearance searches, which show an excess of signal-like events at low reconstructed neutrino energies, with respect to the expected background. A significant component of this background comes from photon emission induced by (anti)neutrino neutral current interactions with nucleons and nuclei. With an improved microscopic model for these reactions, we predict the number and distributions of photon events at the MiniBooNE detector. Our results are compared to the MiniBooNE in situ estimate and to other theoretical approaches. We find that, according to our model, neutral current photon emission fro…

Particle physicsNuclear and High Energy PhysicsPhotonNuclear TheoryFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsMiniBooNENuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsNeutral current010308 nuclear & particles physicsFísicaSolar neutrino problemlcsh:QC1-999High Energy Physics - PhenomenologyPhoton emissionHigh Energy Physics::ExperimentNeutrinoNucleonlcsh:Physics
researchProduct

Sensitivities to neutrino electromagnetic properties at the TEXONO experiment

2015

18 pages.- 4 figures.- 1 table

Particle physicsNuclear and High Energy PhysicsQuenching factorCoherent elastic neutrino-nucleus scatteringReactor neutrinosPhysics beyond the Standard ModelFOS: Physical sciencesWeak interactionNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Charge radiusNeutrino oscillationPhysicsNeutral currentScatteringFísicalcsh:QC1-999Neutrino magnetic momentHigh Energy Physics - PhenomenologyCoherent elastic neutrino–nucleus scattering (CENNS)Neutrino charge radiusNeutrinoRandom phase approximationWeak mixing anglelcsh:PhysicsPhysics Letters B
researchProduct

Bilinear R-parity violation with flavor symmetry

2012

Bilinear R-parity violation (BRPV) provides the simplest intrinsically supersymmetric neutrino mass generation scheme. While neutrino mixing parameters can be probed in high energy accelerators, they are unfortunately not predicted by the theory. Here we propose a model based on the discrete flavor symmetry Lambda(4) with a single R-parity violating parameter, leading to (i) correct Cabbibo mixing given by the Gatto-Sartori-Tonin formula, and a successful unification-like b-tau mass relation, and (ii) a correlation between the lepton mixing angles theta(13) and theta(23) in agreement with recent neutrino oscillation data, as well as a (nearly) massless neutrino, leading to absence of neutri…

Particle physicsNuclear and High Energy PhysicsSupersymmetric Standard ModelFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)R-parityDouble beta decay0103 physical sciencesDiscrete and Finite SymmetriesNeutrino Physics010306 general physicsNeutrino oscillationMixing (physics)Physics010308 nuclear & particles physicsComputer Science::Information RetrievalMass generationHigh Energy Physics::PhenomenologyFísicaMassless particleHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Beyond Standard ModelHigh Energy Physics::ExperimentNeutrinoLepton
researchProduct

Measurement of the $\nu_{\mu}$ charged current quasi-elastic cross-section on carbon with the T2K on-axis neutrino beam

2015

17 pages.- 21 figures

Particle physicsNuclear and High Energy Physicschemistry.chemical_elementPion productionAstronomy & AstrophysicsMASSNeutrino beamPION-PRODUCTION7. Clean energy01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentNuclear physicsScatteringCross section (physics)0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron010306 general physicsNeutrino oscillationNuclear Experiment0206 Quantum PhysicsCharged currentPhysicsScience & Technologyhep-ex010308 nuclear & particles physicsScatteringPhysicsDetectorNuclear & Particles PhysicsMODEL0201 Astronomical And Space ScienceschemistryPhysical SciencesHigh Energy Physics::ExperimentNeutrinoCarbonNuclear targets
researchProduct

Conditions for statistical determination of the neutrino mass spectrum in radiative emission of neutrino pairs in atoms

2016

The photon spectrum in macrocoherent atomic de-excitation via radiative emission of neutrino pairs (RENP) has been proposed as a sensitive probe of the neutrino mass spectrum, capable of competing with conventional neutrino experiments. In this paper we revisit this intriguing technique in order to quantify the requirements for statistical determination of some of the properties of the neutrino spectrum, in particular the neutrino mass scale and the mass ordering. Our results are sobering. We find that, even under ideal conditions, the determination of neutrino parameters needs experimental live times of the order of days to years for several laser frequencies, assuming a target of volume o…

Particle physicsPhotonNeutrino theory of lightPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRadiative transferNeutrinsNeutrinos010306 general physicsNeutrino oscillationPhysicsPhotons010308 nuclear & particles physicsSolar neutrino problem3. Good healthFotonsHigh Energy Physics - PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
researchProduct

Phenomenology of scotogenic scalar dark matter

2020

We reexamine the minimal Singlet + Triplet Scotogenic Model, where dark matter is the mediator of neutrino mass generation. We assume it to be a scalar WIMP, whose stability follows from the same $\mathbb{Z} _{2}$ symmetry that leads to the radiative origin of neutrino masses. The scheme is the minimal one that allows for solar and atmospheric mass scales to be generated. We perform a full numerical analysis of the signatures expected at dark matter as well as collider experiments. We identify parameter regions where dark matter predictions agree with theoretical and experimental constraints, such as neutrino oscillations, Higgs data, dark matter relic abundance and direct detection searche…

Particle physicsPhysics and Astronomy (miscellaneous)Dark matterScalar (mathematics)FOS: Physical scienceslcsh:AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital Libraries7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNeutrino oscillationEngineering (miscellaneous)Light dark matterPhysics010308 nuclear & particles physicsMass generationHigh Energy Physics - PhenomenologyComputer Science::Mathematical SoftwareHiggs bosonlcsh:QC770-798High Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)
researchProduct

Constraining the nonstandard interaction parameters in long baseline neutrino experiments

2016

In this article we investigate the prospects for probing the strength of the possible non-standard neutrino interactions (NSI) in long baseline neutrino oscillation experiments. We find that these experiments are sensitive to NSI couplings down to the level of 0.01-0.1 depending on the oscillation channel and the baseline length, as well as on the detector's fiducial mass. We also investigate the interference of the leptonic CP angle $\delta_{CP}$ with the constraining of the NSI couplings. It is found that the interference is strong in the case of the $\nu_{e}\leftrightarrow\nu_{\mu}$ and $\nu_{e}\leftrightarrow\nu_{\tau}$ transitions but not significant in other transitions. In our numeri…

Particle physicsPhysics beyond the Standard ModelFOS: Physical sciences114 Physical sciences01 natural sciencesOSCILLATION EXPERIMENTSNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)EXPERIMENT-SIMULATOR0103 physical sciencesneutrino oscillationStatistical analysisSensitivity (control systems)010306 general physicsNeutrino oscillationlong baseline experimentsPhysicsta114010308 nuclear & particles physicsOscillationHigh Energy Physics::Phenomenologynonstandard neutrino interactionsneutriino-oskillaatioHigh Energy Physics - PhenomenologyCP violationHigh Energy Physics::ExperimentATMOSPHERIC NEUTRINOSNeutrinoPhysical Review D
researchProduct