Search results for "neutrino oscillation"

showing 10 items of 521 documents

Neutrino physics from cosmological observables and oscillation experiments

2018

Aquesta tesi se centra en la física dels neutrins. En particular, se centra en l'estudi de les oscil·lacions de sabor, el paper dels neutrins relíquia en alguns escenaris cosmològics i la interacció entre aquests dos temes. Els neutrins es troben entre les partícules elementals més conegudes. Presenten comportaments interessants, com les seves oscil·lacions, i constitueixen un dels vincles entre les diferents àrees de la física. A través d'aquest document explotem la seva relació amb la cosmologia, amb especial èmfasi en l'Univers primerenc, encara que també parlem de projectes relacionats amb les últimes etapes de la història de l'Univers. En la primera part de la tesi presentem un ajustam…

neutrino oscillations:FÍSICA [UNESCO]UNESCO::FÍSICAparticle physicsneutrino cosmology
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Interplay between collective effects and non-standard interactions of supernova neutrinos

2009

We consider the effect of nonstandard neutrino interactions (NSI, for short) on the propagation of neutrinos through the supernova (SN) envelope within a three-neutrino framework and taking into account the presence of a neutrino background. We find that for given NSI parameters, with strength generically denoted by epsilon(ij), neutrino evolution exhibits a significant time dependence. For vertical bar epsilon(tau tau)vertical bar greater than or similar to 10(-3) the neutrino survival probability may become sensitive to the V-23 octant and the sign of epsilon(tau tau). In particular, if epsilon(tau tau) greater than or similar to 10(-2) an internal I-resonance may arise independently of t…

PhysicsNuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesElementary particleFermionMassless particleSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorAstrophysics - Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationSolar and Stellar Astrophysics (astro-ph.SR)Lepton
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Measuring the leptonic CP phase in neutrino oscillations with nonunitary mixing

2017

Non-unitary neutrino mixing implies an extra CP violating phase that can fake the leptonic Dirac CP phase $\delta_{CP}$ of the simplest three-neutrino mixing benchmark scheme. This would hinder the possibility of probing for CP violation in accelerator-type experiments. We take T2K and T2HK as examples to demonstrate the degeneracy between the "standard" (or "unitary") and "non-unitary" CP phases. We find, under the assumption of non-unitary mixing, that their CP sensitivities severely deteriorate. Fortunately, the TNT2K proposal of supplementing T2(H)K with a $\mu$DAR source for better measurement of $\delta_{CP}$ can partially break the CP degeneracy by probing both $\cos \delta_{CP}$ and…

PhysicsParticle physicsUnitarity010308 nuclear & particles physicsFOS: Physical sciencesUnitary state01 natural sciencesPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Violació CP (Física nuclear)0103 physical sciencesCP violationStatistical analysisNeutrino010306 general physicsDegeneracy (mathematics)Neutrino oscillation
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Hunt for θ13with LENA

2012

In a hunt for by far missing neutrino mixing angle ?13 the accelerator experiments have recently indicated non-zero value and the dedicated reactor neutrino experiments are moving towards the data-taking phase to confirm that. The small effect of ?13 to the neutrino oscillation probabilities can be also complementarily probed using artificially made source of mono-chromatic neutrinos with low energies originated from electron capture processes. Due to the small energy of neutrino and tiny interaction cross section, and the expected scale of ?13 support the use of large liquid scintillation detector. In this work, the estimated sensitivities for measurement of mixing angle ?13 is presented i…

PhysicsHistorySterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoHigh Energy Physics::PhenomenologySolar neutrino problemComputer Science ApplicationsEducationNuclear physicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNeutrino oscillationJournal of Physics: Conference Series
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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
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Neutrino oscillations and new physics

2005

I discuss the theoretical background and the status of neutrino oscillation parameters from the current worlds' global data sample and latest flux calculations. I give their allowed ranges, best fit values and discuss the small parameters and sin2theta13, which characterize CP violation in neutrino oscillations. I mention the significance of neutrinoless double beta decay and current expectations in view of oscillation results.

PhysicsNuclear and High Energy PhysicsParticle physicsOscillationPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFluxFOS: Physical sciencesFísicaAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Double beta decayCP violationHigh Energy Physics::ExperimentNeutrino oscillation
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Neutrino oscillation parameters: Future

2019

The Neutrino Oscillation Workshop (NOW2018) included a session addressing neutrino oscillation parameters in the future. This session included discussion of planned and proposed experiments, detector technologies, and analysis techniques to better measure neutrino oscillation parameters. Constraint of systematic uncertainty in future precision measurements was a topic of particular interest. This proceedings is a brief summary of the presentations in the Oscillation Parameters: Future session; readers are directed to individual contributions to the proceedings for more detailed information.

Systematic errorConstraint (information theory)Particle physicsOscillationComputer scienceDetectorMeasure (physics)High Energy Physics::ExperimentSession (computer science)Neutrino oscillationPartícules (Física nuclear)
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Pulsar Velocities without Neutrino Mass

1998

We show that pulsar velocities may arise from anisotropic neutrino emission induced by resonant conversions of massless neutrinos in the presence of a strong magnetic field. The main ingredient is a small violation of weak universality and neither neutrino masses nor magnetic moments are required.

PhysicsNuclear and High Energy PhysicsParticle physicsMagnetic momentPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)General Physics and AstronomyFísicaFOS: Physical sciencesElementary particleSolar neutrino problemAstrophysicsAtomic and Molecular Physics and OpticsMagnetic fieldMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)PulsarMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLepton
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A high precision calorimeter for hunting the sterile neutrino in the SOX experiment

2019

Abstract A thermal calorimetric apparatus was designed, built and calibrated for measuring the activity of the artificial 144 Ce —144 Pr antineutrino source. This measurement will be performed at the Laboratori Nazionali del Gran Sasso in Italy, just before the source insertion in the tunnel under the Borexino detector and a precision better than 1% is required for a disappearance technique measurement in the SOX (Short distance neutrino Oscillation with BoreXino) project. In this work the apparatus is described and the most important results from the calibration measurements are shown, where the final precision of few per thousand is demonstrated.

PaperPhysicsHistorySterile neutrinoDetectorddc:Computer Science ApplicationsEducationShort distanceCalorimeterNuclear physicsThermalCalibrationNeutrino oscillationBorexino
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Genuine and Matter-induced Components of the CPV Asymmetry for Neutrino Oscillations

2019

These results represent the solution for the historical problem of the contamination by matter effects on the CPV Asymmetry for neutrino oscillations. Vacuum is CPT-symmetric and matter is T-symmetric, the goal is accomplished by using this guiding principle. Independent of the theoretical framework for the dynamics of the active neutrino flavors, we prove the Disentanglement Theorem A(CP)=A(CP, T)+A(CP, CPT) for the experimental CPV Asymmetry, with A(CP, T) genuine T-odd and A(CP, CPT) fake CPT-odd. For the effective Hamiltonian written as the sum of free mass propagation plus the matter potential for electron-neutrinos, the two components have definite parities under the baseline L, the m…

PhysicsParticle physicsOscillationmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyZero (complex analysis)FOS: Physical sciencesAsymmetryHigh Energy Physics - Phenomenologysymbols.namesakeMatrix (mathematics)High Energy Physics - Phenomenology (hep-ph)symbolsHigh Energy Physics::ExperimentNeutrinoHamiltonian (quantum mechanics)Neutrino oscillationSign (mathematics)media_common
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