Search results for "Neutrino ma"

showing 10 items of 55 documents

Structure and prospects of the simplest SO(10) GUTs

2012

We recapitulate the latest results on the class of the simplest SO(10) grand unified models in which the GUT-scale symmetry breaking is triggered by an adjoint Higgs representation. We argue that the minimal survival approximation traditionally used in the GUT- and seesaw-scale estimates tends to be blind to very interesting parts of the parameter space in which some of the intermediate-scale states necessary for non-supersymmetric unification of the SM gauge couplings can be as light as to leave their imprints in the TeV domain. The stringent minimal-survival-based estimates of the B-L scale are shown to be relaxed by as much as four orders of magnitude, thus admitting for a consistent imp…

PhysicsParticle physicsSO(10)010308 nuclear & particles physicsProton decayHigh Energy Physics::PhenomenologyGrand unification; Neutrino masses; SO(10)Structure (category theory)FOS: Physical sciencesNeutrino massesParameter space01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw mechanismOrders of magnitude (time)Grand unification0103 physical sciencesHiggs bosonSymmetry breakingSO(10)010306 general physics
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Quark-lepton mass relation and CKM mixing in an A(4) extension of the minimal supersymmetric standard model

2013

An interesting mass relation between down-type quarks and charged leptons has been recently predicted within a supersymmetric SU(3)(c) circle times SU(2)(L) circle times U(1)(Y) model based on the A(4) flavor symmetry. Here we propose a simple extension which provides an adequate full description of the quark sector. By adding a pair of vectorlike up quarks, we show how the CKM entries V-ub, V-cb, V-td and V-ts arise from deviations of the unitarity. We perform an analysis including the most relevant observables in the quark sector, such as oscillations and rare decays of kaons, B-d and B-s mesons. In the lepton sector, the model predicts an inverted hierarchy for the neutrino masses, leadi…

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsMesonUnitarity010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixPhysics beyond the Standard ModelHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSupersymmetryNeutrino masses01 natural sciencesHigh Energy Physics - PhenomenologySymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesUp quarkHigh Energy Physics::Experiment010306 general physicsLepton
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Neutrinoless double β decay with small neutrino masses

2013

Proceedings of the Corfu Summer Institute 2012 "School and Workshops on Elementary Particle Physicsand Gravity", September 8-27, 2012, Corfu (Greece). PoS(Cofu2012)028.

PhysicsQuarkParticle physicsPhysics beyond the Standard ModelDouble betaHigh Energy Physics::PhenomenologyFísicaNeutrinolessLepton numberPartícules (Física nuclear)Operator (computer programming)Neutrino massDouble beta decayHigh Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)LeptonDouble β
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Working group report: Neutrino physics

2009

This is the report of the neutrino physics working group at WHEPP-X. We summarize the problems selected and discussed at the workshop and the papers which have resulted subsequently.

Physicsline-experiment-simulatorParticle physicsGroup (mathematics)Solar neutrinooscillation experimentsGeneral Physics and AstronomyNeutrino Mass ModelsSolar neutrino problemPhysics and Astronomy(all)Oscillation ExperimentsNeutrino OscillationsNuclear physicsLeptogenesisLine-Experiment-SimulatorLeptogenesisPhysical Sciences and MathematicsMeasurements of neutrino speedNeutrinoLepton Flavour ViolationNeutrino oscillation
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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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Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

2018

The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, and its determination may provide the key to establish the relationship among the lepton masses and mixings and their analogous properties in the quark sector. The extraction of the neutrino mass ordering is a data-driven field expected to evolve very rapidly in the next decade. In this review, we both analyze the present status and describe the physics of subsequent prospects. Firstly, the different current available tools to measure the neutrino mass ordering are described. Namely, reactor, long-baseline (accelerator and atmospheric) neutrino beams, laboratory searches for beta and neutrinol…

QuarkParticle physicsneutrino masses and flavor mixingCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)lcsh:AstronomyCosmic background radiationneutrino mass orderingFOS: Physical scienceslarge scale structure formation7. Clean energy01 natural sciencesCosmologyPartícules (Física nuclear)lcsh:QB1-991High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino oscillation010303 astronomy & astrophysicsPhysicsneutrino oscillations010308 nuclear & particles physicslcsh:QC801-809High Energy Physics::Phenomenologyneutrinoless double beta (0vββ) decayAstronomy and AstrophysicsHigh Energy Physics - PhenomenologySupernovalcsh:Geophysics. Cosmic physicscosmic microwave Background (CMB)High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsLeptonFrontiers in Astronomy and Space Sciences
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Reduction of stored-particle background by a magnetic pulse method at the KATRIN experiment

2018

Arenz, M., et al. “Reduction of Stored-Particle Background by a Magnetic Pulse Method at the KATRIN Experiment.” The European Physical Journal C, vol. 78, no. 9, Sept. 2018. © 2018 The Authors

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Field (physics)Physics::Instrumentation and DetectorsFOS: Physical scienceslcsh:AstrophysicsElectronKATRIN01 natural sciencesradon: nuclideNeutrino mass0103 physical scienceslcsh:QB460-466coillcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsnumerical calculationsEngineering (miscellaneous)background: radioactivitybackground: suppressionPhysicsSpectrometer010308 nuclear & particles physicsPhysicsOrder (ring theory)Monte Carlo methodsInstrumentation and Detectors (physics.ins-det)Radon backgroundPulse (physics)13. Climate actionBackground reduction methodsPartículaslcsh:QC770-798spectrometerAtomic physicsElectricidadElectron neutrinoKATRIN
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Suppression of Penning discharges between the KATRIN spectrometers

2020

The KArlsruhe TRItium Neutrino experiment (KATRIN) aims to determine the effective electron (anti)neutrino mass with a sensitivity of $0.2\textrm{ eV/c}^2$ (90$\%$ C.L.) by precisely measuring the endpoint region of the tritium $\beta$-decay spectrum. It uses a tandem of electrostatic spectrometers working as MAC-E (magnetic adiabatic collimation combined with an electrostatic) filters. In the space between the pre-spectrometer and the main spectrometer, an unavoidable Penning trap is created when the superconducting magnet between the two spectrometers, biased at their respective nominal potentials, is energized. The electrons accumulated in this trap can lead to discharges, which create a…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsPenning trapFOS: Physical scienceslcsh:AstrophysicsSuperconducting magnetElectronTritiumKATRIN01 natural sciencesNuclear physics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectron Captureddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentEngineering (miscellaneous)PhysicsSpectrometer010308 nuclear & particles physicsPhysicsInstrumentation and Detectors (physics.ins-det)Químicamagnet: superconductivityspectrometer: electrostaticPenning trapBeamlineBeta (plasma physics)electron: backgroundlcsh:QC770-798NeutrinoNeutrino MassKATRIN
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Cosmic microwave background constraints on secret interactions among sterile neutrinos

2017

Secret contact interactions among eV sterile neutrinos, mediated by a massive gauge boson $X$ (with $M_X \ll M_W$), and characterized by a gauge coupling $g_X$, have been proposed as a mean to reconcile cosmological observations and short-baseline laboratory anomalies. We constrain this scenario using the latest Planck data on Cosmic Microwave Background anisotropies, and measurements of baryon acoustic oscillations (BAO). We consistently include the effect of secret interactions on cosmological perturbations, namely the increased density and pressure fluctuations in the neutrino fluid, and still find a severe tension between the secret interaction framework and cosmology. In fact, taking i…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosDark matterCosmic microwave backgroundFOS: Physical sciencescosmological neutrinos; cosmological parameters from CMBR; neutrino masses from cosmology; neutrino properties; Astronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNOsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsneutrino propertiesPhysicsGauge bosoncosmological neutrino010308 nuclear & particles physicsHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and Astrophysicsneutrino masses from cosmologyCoupling (probability)3. Good healthHigh Energy Physics - Phenomenology13. Climate actionsymbolsHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments

2020

The current and upcoming generation of Very Large Volume Neutrino Telescopes – collecting unprecedented quantities of neutrino events – can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as M…

data analysis methodNuclear and High Energy PhysicsMonte Carlo methodFVLV nu TData analysis; Detector; KDE; MC; Monte Carlo; Neutrino; Neutrino mass ordering; Smoothing; Statistics; VLVνTData analysisKDEFOS: Physical sciences01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)statistical analysisnumerical methods0103 physical sciencesStatisticsNeutrinoddc:530Sensitivity (control systems)MC010306 general physicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMonte CarloPhysicsVLVνT010308 nuclear & particles physicsOscillationStatisticsoscillation [neutrino]ObservableDetectorMonte Carlo [numerical calculations]WeightingNeutrino mass orderingPhysics and AstronomyPhysics - Data Analysis Statistics and ProbabilityPhysique des particules élémentairesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsMATTERData Analysis Statistics and Probability (physics.data-an)SmoothingSmoothing
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