Search results for "neutrino mass"

showing 10 items of 53 documents

Electroweak breaking and neutrino mass

2017

En este trabajo de tesis hemos analizado algunas de las posibles conexiones entre la generación de la masa de los neutrinos y la nueva física. Para ello, como preámbulo, en el primer capítulo hemos hecho un repaso del Modelo Estándar (SM) de la física de partículas, siendo ésta la descripción más precisa que tenemos de las las interacciones fuertes, débiles y electromagnéticas. Sin embargo, existen algunas interrogantes a las que el SM no ofrece respuesta, por ejemplo, ¿Por qué hay tres familias de quarks y leptones?, ¿Cuál es la explicación a la jerarquía de las masas de los fermiones y a sus ángulos de mezcla?, ¿Cómo explicar la jerarquía entre la escala electrodébil y la escala de Planck…

Neutrino massneutrino natureHiggs propertiesdark matterFlavour symmetries
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Neutrinoless ββ decays to excited 0+ states and the Majorana-neutrino mass

2016

The nuclear matrix elements (NMEs) corresponding to the neutrinoless double-β (0νββ) decays to excited 0+ states of major experimental interest are calculated. All these decay transitions are electron emitting (0νβ−β− decays) and take place in the mass A = 76,82,96,100,110,116,124,130,136 nuclei. This work is an extension of our previous work [Phys. Rev. C 91, 024613 (2015)], where 0νββ decays to the ground states of the same nuclei were treated. We calculate the NMEs for transitions mediated by both the light (l-NMEs) and the heavy (h-NMEs) Majorana neutrinos. A higher-QRPA (quasiparticle random-phase approximation) framework, the multiple-commutator model, is adopted for the calculations,…

Nuclear TheoryMajorana-neutrino massnuclear matrix elementsfysiikkaNuclear Experiment
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Role of dense matter in collective supernova neutrino transformations

2008

6 pages, 2 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ArXiv pre-print available at: http://arxiv.org/abs/0807.0659

Nuclear and High Energy PhysicsElectron densityParticle physicsQuantum decoherenceNeutrino mass and mixing[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Critical phenomenaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] SupernovaeAstrophysics[PACS] Neutrino mass and mixingAstrophysics01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísica3. Good healthSupernovaHigh Energy Physics - PhenomenologySupernovae14.60.Pq 97.60.Bw[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentNeutrinoEarly phaseDense matter
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Neutrino phenomenology and stable dark matter with A4

2011

We present a model based on the A4 non-abelian discrete symmetry leading to a predictive five-parameter neutrino mass matrix and providing a stable dark matter candidate. We found an interesting correlation among the atmospheric and the reactor angles which predicts theta_23 ~ pi/4 for very small reactor angle and deviation from maximal atmospheric mixing for large theta_13. Only normal neutrino mass spectrum is possible and the effective mass entering the neutrinoless double beta decay rate is constrained to be |m_ee| > 4 10^{-4} eV.

Nuclear and High Energy PhysicsParticle physicsLepton mixingDark matterDiscrete symmetriesFOS: Physical sciencesElementary particle01 natural sciences7. Clean energyNuclear physicsEffective mass (solid-state physics)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesDark matterNeutrinoless double beta decay010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsFlavor symmetriesNeutrino massesMassless particleHigh Energy Physics - PhenomenologyMass spectrumNeutrinoPhysics Letters B
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Admixture of quasi-Dirac and Majorana neutrinos with tri-bimaximal mixing

2011

7 páginas, 1 tabla.-- El Pdf es la versión pre-print: arXiv:1104.4961v2

Nuclear and High Energy PhysicsParticle physicsNeutrino hierarchyDiscrete symmetriesFOS: Physical sciences01 natural sciencesUpper and lower boundsHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesTri-bimaximal mixingNeutrino masses and mixingsNeutrinoless double beta decay010306 general physicsMixing (physics)Majorana equationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFlavor symmetries3. Good healthMassless particleMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoLepton
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Exact relativistic beta decay endpoint spectrum

2007

5 pages, 3 figures.-- PACS nrs.: 14.60.Pq; 13.30.-a; 23.40.-s; 23.40.Bw.-- ISI Article Identifier: 000250620900070.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.0897

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciences[PACS] Neutrino mass and mixingelectron and muon captureHigh Energy Physics - Phenomenology (hep-ph)FactorizationDouble beta decayNuclear Experiment (nucl-ex)Neutrino oscillationNuclear ExperimentPhysics[PACS] β decay[PACS] Decays of baryonsSpectrum (functional analysis)[PACS] β decay; double β decay; electron and muon captureFísicaBeta decay[PACS] Weak-interaction and lepton (including neutrino) aspects of β decayHigh Energy Physics - Phenomenologydouble β decayYield (chemistry)High Energy Physics::ExperimentNeutrinoKATRIN
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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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Flavored CP asymmetries for type II seesaw leptogenesis

2013

A novel contribution to the leptonic CP asymmetries in type II seesaw leptogenesis scenarios is obtained for the cases in which flavor effects are relevant for the dynamics of leptogenesis. In the so-called flavored leptogenesis regime, the interference between the tree-level amplitude of the scalar triplet decaying into two leptons and the one-loop wave function correction with leptons in the loop, leads to a new nonvanishing CP asymmetry contribution. The latter conserves total lepton number but violates lepton flavor. Cases in which this novel contribution may be dominant in the generation of the baryon asymmetry are briefly discussed.

Nuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectFlavourScalar (mathematics)FOS: Physical sciences01 natural sciencesAsymmetryHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetrySeesaw molecular geometryModels0103 physical sciences010306 general physicsmedia_commonPhysicsViolation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyBaryogenesisFísicaAstronomy and AstrophysicsNeutrino MassesLepton numberAtomic and Molecular Physics and OpticsTripletMixingsNeutrino physicsHigh Energy Physics - PhenomenologyGaugeLeptogenesisLeptogenesisSeesaw mechanismHigh Energy Physics::ExperimentLepton
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A design for an electromagnetic filter for precision energy measurements at the tritium endpoint

2019

We present a detailed description of the electromagnetic filter for the PTOLEMY project to directly detect the Cosmic Neutrino Background (CNB). Starting with an initial estimate for the orbital magnetic moment, the higher-order drift process of E×B is configured to balance the gradient-B drift motion of the electron in such a way as to guide the trajectory into the standing voltage potential along the mid-plane of the filter. As a function of drift distance along the length of the filter, the filter zooms in with exponentially increasing precision on the transverse velocity component of the electron kinetic energy. This yields a linear dimension for the total filter length that is exceptio…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsFOS: Physical sciencesElectron7. Clean energy01 natural sciencesPartícules (Física nuclear)Hamiltonian systemNeutrino massRelic neutrino0103 physical sciencesTransverse drift filter010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PTOLEMYPhysicsMagnetic moment010308 nuclear & particles physicsCNB; Cosmic Neutrino Background; Neutrino mass; PTOLEMY; Relic neutrino; Transverse drift filterInstrumentation and Detectors (physics.ins-det)CNBFilter (signal processing)CNB; Cosmic Neutrino Background; Neutrino mass; PTOLEMY; Relic neutrino; Transverse drift filter; Nuclear and High Energy PhysicsComputational physicsEnergy conservationHarmonicAstrophysics - Instrumentation and Methods for AstrophysicsNeutrino maEnergy (signal processing)Cosmic Neutrino BackgroundVoltageProgress in Particle and Nuclear Physics
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High-resolution spectroscopy of gaseous $^\mathrm{83m}$Kr conversion electrons with the KATRIN experiment

2020

In this work, we present the first spectroscopic measurements of conversion electrons originating from the decay of metastable gaseous $^\mathrm{83m}$Kr with the Karlsruhe Tritium Neutrino (KATRIN) experiment. The results obtained in this calibration measurement represent a major commissioning milestone for the upcoming direct neutrino mass measurement with KATRIN. The successful campaign demonstrates the functionalities of the full KATRIN beamline. The KATRIN main spectrometer's excellent energy resolution of ~ 1 eV made it possible to determine the narrow K-32 and L$_3$-32 conversion electron line widths with an unprecedented precision of ~ 1 %.

Nuclear and High Energy PhysicsSpeichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsResolution (mass spectrometry)Physics::Instrumentation and Detectorsenergy resolutionFOS: Physical sciencesElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]KATRIN7. Clean energy01 natural sciencesAtomicneutrino massNuclear physicsParticle and Plasma Physicsconversion electronsMetastability0103 physical sciencesNuclearddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsSpectroscopyNuclear ExperimentPhysicsSpectrometerelectrostatic spectrometer010308 nuclear & particles physicsPhysicskrypton: decayMolecularInstrumentation and Detectors (physics.ins-det)krypton: nuclide530 PhysikcalibrationNuclear & Particles Physicsddc:3. Good healthBeamlineelectron: energy spectrumNeutrinoperformanceKATRIN
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