Search results for "Neutrino Mass"

showing 10 items of 53 documents

Supersymmetric SO(10)-inspired GUTs with sliding scales

2013

We construct lists of supersymmetric models with extended gauge groups at intermediate steps, all of which are inspired by SO(10) unification. We consider three different kinds of setups: (i) the model has exactly one additional intermediate scale with a left-right (LR) symmetric group; (ii) SO(10) is broken to the LR group via an intermediate Pati-Salam scale; and (iii) the LR group is broken into SU(3)(c) X SU(2)(L) X U(1)(R) X U(1)(B-L), before breaking to the standard model (SM) group. We use sets of conditions, which we call the "sliding mechanism," which yield unification with the extended gauge group(s) allowed at arbitrary intermediate energy scales. All models thus can have new gau…

Left-right symmetryNeutrino massModelsUnificationHigh Energy Physics::PhenomenologyGrand unified theoryNumberFísicaHiggs-bosonR-ParityBreakingLeptons
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High-precision electron-capture Q value measurement of 111In for electron-neutrino mass determination

2022

A precise determination of the ground state $^{111}$In ($9/2^+$) electron capture to ground state of $^{111}$Cd ($1/2^+$) $Q$ value has been performed utilizing the double Penning trap mass spectrometer, JYFLTRAP. A value of 857.63(17) keV was obtained, which is nearly a factor of 20 more precise than the value extracted from the Atomic Mass Evaluation 2020 (AME2020). The high-precision electron-capture $Q$ value measurement along with the nuclear energy level data of 866.60(6) keV, 864.8(3) keV, 855.6(10) keV, and 853.94(7) keV for $^{111}$Cd was used to determine whether the four states are energetically allowed for a potential ultra-low $Q$-value $\beta^{}$ decay or electron-capture deca…

Nuclear and High Energy PhysicsmassaspektrometriaNeutrino massUltra-low Q valueAstrophysics::High Energy Astrophysical PhenomenaPenning trapneutriinotFOS: Physical sciencesNuclear Experiment (nucl-ex)ydinfysiikkaNuclear ExperimentMass measurementsElectron capturePhysics Letters B
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High-precision measurement of a low Q value for allowed β−-decay of 131I related to neutrino mass determination

2022

The ground-state-to-ground-state β−-decay 131I (7/2+) → 131Xe (3/2+) Q value was determined with high precision utilizing the double Penning trap mass spectrometer JYFLTRAP at the IGISOL facility. The Q value of this β−-decay was found to be Q = 972.25(19) keV through a cyclotron frequency ratio measurement with a relative precision of 1.6 × 10−9. This was realized using the phase-imaging ion-cyclotron-resonance technique. The new Q value is more than 3 times more precise and 2.3σ higher (1.45 keV) than the value extracted from the Atomic Mass Evaluation 2020. Our measurement confirms that the β−-decay to the 9/2+ excited state at 971.22(13) keV in 131Xe is energetically allowed with a Q va…

β− decayNuclear and High Energy PhysicsScience & TechnologyPhysicsPenning trapLow Q valuebeta(-) decayneutriinotAstronomy & AstrophysicsERRORSPhysics Particles & FieldsPhysics NuclearNeutrino massNUCLEAR-DATA SHEETSPhysical SciencesJYFLTRAPBETA-DECAYydinfysiikkaPhysics Letters B
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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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Non-standard interactions: Atmospheric versus neutrino factory experiments

2001

We consider the potential of a generic neutrino factory (NUFACT) in probing non-standard neutrino-matter interactions (NSI). We find that the sensitivity to flavour-changing (FC) NSI can be substantially improved with respect to present atmospheric neutrino data, especially at energies higher than approximately 50 GeV, where the effect of the tau mass is small. For example, a 100 GeV NUFACT can probe FC neutrino interactions at the level of few $|\epsilon| < {few} \times 10^{-4}$ at 99 % C.L.

PhysicsParticle physicsAtmospheric neutrinosNuclear and High Energy PhysicsNeutrino mass and mixingNeutrino oscillationsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNeutrino factoryFOS: Physical sciencesFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino FactoryHigh Energy Physics::ExperimentSensitivity (control systems)Atmospheric neutrinoNeutrino
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Decoherence in supernova neutrino transformations suppressed by deleptonization

2007

16 pages, 12 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ISI Article Identifier: 000251987300100.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.2498

HistoryParticle physicsNuclear and High Energy PhysicsQuantum decoherence[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] Supernovae[PACS] Neutrino mass and mixingAstrophysicsAsymmetryMeasure (mathematics)01 natural sciences7. Clean energyEarly UniverseStandard ModelEducationLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesInvariant massddc:530High Energy Physics010306 general physicsMixing (physics)media_commonPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaWeinberg angleFunction (mathematics)Atomic and Molecular Physics and OpticsComputer Science Applications3. Good healthSupernovaHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentNeutrino
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Production, isolation and characterization of radiochemically pure 163Ho samples for the ECHo-project

2018

Abstract Several experiments on the study of the electron neutrino mass are based on high-statistics measurements of the energy spectrum following electron capture of the radionuclide 163Ho. They rely on the availability of large, radiochemically pure samples of 163Ho. Here, we describe the production, separation, characterization, and sample production within the Electron Capture in Holmium-163 (ECHo) project. 163Ho has been produced by thermal neutron activation of enriched, prepurified 162Er targets in the high flux reactor of the Institut Laue-Langevin, Grenoble, France, in irradiations lasting up to 54 days. Irradiated targets were chemically processed by means of extraction chromatogr…

ChromatographyChemistryEcho (computing)lanthanide separationneutron activation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]010403 inorganic & nuclear chemistryIsolation (microbiology)7. Clean energy01 natural sciencesNeutrino mass determination0104 chemical sciencesCharacterization (materials science)163Ho0103 physical sciencesextraction chromatographyPhysical and Theoretical Chemistry010306 general physicsNeutron activationRadiochimica Acta
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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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Review of Particle Physics

2020

The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, …

high energyleptonmixing [neutrino]High Energy Physics::LatticeCosmic microwave backgrounddiffractionTechnicolorAstrophysicsOmega01 natural sciencesPhysics Particles & Fieldshiggs-boson productionBig Bang nucleosynthesiscosmological model: parameter spacetaudark energyMonte CarlofieldspentaquarkinstrumentationSettore FIS/01gauge bosonAnomalous magnetic dipole momentdeep-inelastic scatteringnew physicsPhysicsDOUBLE-BETA-DECAYElectroweak interactiondensity [dark matter]HEAVY FLAVOURQuarkoniumreview; particle; physicsSUPERSYMMETRIC STANDARD MODELsquare-root-sPhysics Nucleargrand unified theoryboson: heavystatisticsPhysical SciencesHiggs bosonaxion: massflavor: violationNeutrinoELECTROWEAK SYMMETRY-BREAKINGnumerical calculations: Monte Carlophysicson-lineS013EPHQuarkheavy [boson]particle[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Physics Multidisciplinaryanomalous magnetic-momentelectroweak radiative-correctionsdark matter: densityHiggs particlemesonneutrino masses neutrino mixing; neutrino oscillations114 Physical sciencesCHIRAL PERTURBATION-THEORYneutrino mixingStandard Modelquark0202 Atomic Molecular Nuclear Particle And Plasma PhysicsNucleosynthesisquantum chromodynamicsCP: violationDark matterddc:530particle physicsStrong Interactions010306 general physicssparticleS013DFgrand unified theoriesPRODUCTIONGauge bosonScience & Technologyneutrino oscillationsneutrino masses010308 nuclear & particles physicsC50 Other topics in experimental particle physicsParticle Data GroupAstronomy and AstrophysicsDeep inelastic scatteringto-leading-order* Automatic Keywords *heavy bosonaxiontables (particle physics)Tetraquarkproton-proton collisionsSupersymmetryhadronneutrino: mixing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyVolume (compression)HIGGS-BOSONUB-VERTICAL-BARcosmological modeldark energy densityexperimental methodsddc:539.72021Physics beyond the Standard Modelstandard modelgroup theoryGeneral Physics and Astronomytables particle physicshigh energy physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamicsPhysicsenergy: highE Rev 2016[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Settore FIS/01 - Fisica SperimentalephotonSupersymmetryNuclear & Particles Physicsparameter space [cosmological model]dark energy: densityhigh [energy]M013WXfermion-pair productionNuclear and High Energy PhysicsParticle physicsHiggs bosonreviewAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics530dark matterstatistical analysisDouble beta decay0103 physical sciencesconservation lawcold dark-matterTAU LEPTONSAstrophysics::Galaxy AstrophysicstablesDEEP-INELASTIC-SCATTERINGelectroweak interactionHigh Energy Physics::Phenomenology750 GeV diphoton excessPRODUCTION CROSS-SECTIONbaryondensity [dark energy]Physics and AstronomygravitationCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentsupersymmetryMinimal Supersymmetric Standard Model
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Neutrino masses and mixing: a flavour symmetry roadmap

2012

Over the last ten years tri-bimaximal mixing has played an important role in modeling the flavour problem. We give a short review of the status of flavour symmetry models of neutrino mixing. We concentrate on non-Abelian discrete symmetries, which provide a simple way to account for the TBM pattern. We discuss phenomenological implications such as neutrinoless double beta decay, lepton flavour violation as well as theoretical aspects such as the possibility to explain quarks and leptons within a common framework, such as grand unified models

QuarkParticle physicsNuclear TheoryHigh Energy Physics::LatticeFlavourFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesneutrino mixingNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences010306 general physicsMixing (physics)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaNeutrino massesCommon frameworkSymmetry (physics)High Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoflavour symmetryLeptonFortschritte der Physik
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