Search results for "Measurements"

showing 10 items of 720 documents

Global status of neutrino oscillation parameters after Neutrino-2012

2012

Here we update the global fit of neutrino oscillations in arXiv:1103.0734 and arXiv:1108.1376 including the recent measurements of reactor antineutrino disappearance reported by the Double Chooz, Daya Bay and RENO experiments, together with latest MINOS and T2K appearance and disappearance results, as presented at the Neutrino-2012 conference. We find that the preferred global fit value of $\theta_{13}$ is quite large: $\sin^2\theta_{13} \simeq 0.025$ for normal and inverted neutrino mass ordering, with $\theta_{13} = 0$ now excluded at more than 10$\sigma$. The impact of the new $\theta_{13}$ measurements over the other neutrino oscillation parameters is discussed as well as the role of th…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesCHOOZ01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsNOνA010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyMINOSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Mass Varying Neutrinos in the Sun

2005

In this work we study the phenomenological consequences of the dependence of mass varying neutrinos on the neutrino density in the Sun, which we precisely compute in each point along the neutrino trajectory. We find that a generic characteristic of these scenarios is that they establish a connection between the effective Delta m^2 in the Sun and the absolute neutrino mass scale. This does not lead to any new allowed region in the oscillation parameter space. On the contrary, due to this effect, the description of solar neutrino data worsens for large absolute mass. As a consequence a lower bound on the level of degeneracy can be derived from the combined analysis of the solar and KamLAND da…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesParameter spaceAstrophysics01 natural sciences7. Clean energyUpper and lower boundsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsStandard solar model010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaSolar neutrino problemHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Status of global fits to neutrino oscillations

2004

We review the present status of global analyses of neutrino oscillations, taking into account the most recent neutrino data including the latest KamLAND and K2K updates presented at Neutrino2004, as well as state-of-the-art solar and atmospheric neutrino flux calculations. We give the two-neutrino solar + KamLAND results, as well as two-neutrino atmospheric + K2K oscillation regions, discussing in each case the robustness of the oscillation interpretation against departures from the Standard Solar Model and the possible existence of non-standard neutrino physics. Furthermore, we give the best fit values and allowed ranges of the three-flavour oscillation parameters from the current worlds' …

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsStandard solar modelDegree (graph theory)010308 nuclear & particles physicsOscillationAnomaly (natural sciences)Astrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSolar neutrino problemAtomic and Molecular Physics and Opticsddc:High Energy Physics - Phenomenology13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrino
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Updating neutrino magnetic moment constraints

2016

20 pages.- 4 figures.- Addendum on the limit from the Borexino data

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoPhysics beyond the Standard ModelFOS: Physical sciencesElectromagnetic properties01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationMajorana neutrinosBorexinoPhysicsMagnetic moment010308 nuclear & particles physicslcsh:QC1-999High Energy Physics - PhenomenologyNucleus coherent scatteringMeasurements of neutrino speedCP violationBorexinoNeutrinolcsh:Physics
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Dirac neutrinos from flavor symmetry

2013

We present a model where Majorana neutrino mass terms are forbidden by the flavor symmetry group Delta(27). Neutrinos are Dirac fermions and their masses arise in the same way as that of the charged fermions, due to very small Yukawa couplings. The model fits current neutrino oscillation data and correlates the octant of the atmospheric angle with the magnitude of the lightest neutrino mass, with maximal mixing excluded for any neutrino mass

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoNeutrino theory of lightPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::LatticePontecorvo–Maki–Nakagawa–Sakata matrixFOS: Physical sciences7. Clean energy01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyDirac fermionsymbolsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Limits on sterile neutrino contributions to neutrinoless double beta decay

2015

Nuclear matrix elements (NME) for exchange of arbitrary mass neutrinos are calculated in the interacting boson model (IBM-2). By combining the NME with the phase space factors (PSF), expected half-lives for neutrinos of mass ${m}_{N}$ and coupling ${U}_{eN}$ are estimated. Limits on sterile neutrinos with masses in the eV, keV, MeV-GeV, and TeV range are given.

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesdouble beta decaynuclear matrix elements7. Clean energydark matterNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)sterile neutrinosDouble beta decayNuclear ExperimentNeutrino oscillationPhysicsta114High Energy Physics::PhenomenologySolar neutrino problemCoupling (probability)High Energy Physics - PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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Comparative study of electrical behavior and phase transitions in pure and chromium doped α-LiIO3single crystals

1999

Abstract The polymorphic phase transitions of undoped and chromium doped α-LiIO3 crystals have been investigated by means of DTA experiments at slow heating rates and electrical measurements vs temperature and frequency. Upon heating the well known α ⇔ γ ⇒ β sequence appears to be influenced by the sample's morphology, acidity of the growing solution and doping. Dielectric response at room temperature is close to the type “superposition of d.c. ionic conductivity and dipolar response”. We describe the thermal behavior of conductivity along the c polar axis at three frequencies. Electrical measurements also highlight a higher value of ionic conductivity and a less destructive transition for …

Nuclear and High Energy PhysicsPhase transitionRadiationMaterials scienceInorganic chemistryDopingAnalytical chemistrychemistry.chemical_elementLithium iodateConductivityCondensed Matter PhysicsDipoleChromiumchemistry.chemical_compoundchemistryCondensed Matter::SuperconductivityIonic conductivityGeneral Materials ScienceElectrical measurements
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Radiogenic backgrounds in the NEXT double beta decay experiment

2019

[EN] Natural radioactivity represents one of the main backgrounds in the search for neutrinoless double beta decay. Within the NEXT physics program, the radioactivity- induced backgrounds are measured with the NEXT-White detector. Data from 37.9 days of low-background operations at the Laboratorio Subterraneo de Canfranc with xenon depleted in Xe-136 are analyzed to derive a total background rate of (0.84 +/- 0.02) mHz above 1000 keV. The comparison of data samples with and without the use of the radon abatement system demonstrates that the contribution of airborne-Rn is negligible. A radiogenic background model is built upon the extensive radiopurity screening campaign conducted by the NEX…

Nuclear and High Energy PhysicsPhysical measurementsPhysics - Instrumentation and DetectorsDark Matter and Double Beta DecayDark matterFísica -- Mesuramentschemistry.chemical_elementFOS: Physical sciencesRadon7. Clean energy01 natural sciencesAtomicMathematical SciencesHigh Energy Physics - ExperimentNuclear physicsTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)XenonParticle and Plasma PhysicsDouble beta decayDark matter and double beta decay (experiments)0103 physical sciencesDark Matter and Double Beta Decay (experiments)Dark Matterlcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear010306 general physicsDouble Beta DecayNatural radioactivityMathematical PhysicsPhysicsQuantum PhysicsRadiogenic nuclide010308 nuclear & particles physicsDetectorMolecularDetectorsInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicschemistryPhysical Scienceslcsh:QC770-798Event (particle physics)
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Demonstration of the event identification capabilities of the NEXT-White detector

2019

[EN] In experiments searching for neutrinoless double-beta decay, the possibility of identifying the two emitted electrons is a powerful tool in rejecting background events and therefore improving the overall sensitivity of the experiment. In this paper we present the first measurement of the efficiency of a cut based on the different event signatures of double and single electron tracks, using the data of the NEXT-White detector, the first detector of the NEXT experiment operating underground. Using a 228Th calibration source to produce signal-like and background-like events with energies near 1.6 MeV, a signal efficiency of 71.6 ± 1.5 stat ± 0.3 sys% for a background acceptance of 20.6 ± …

Nuclear and High Energy PhysicsPhysical measurementsPhysics - Instrumentation and DetectorsMonte Carlo methodExtrapolationFísica -- MesuramentsFOS: Physical sciences7. Clean energy01 natural sciencesAtomicMathematical SciencesHigh Energy Physics - ExperimentNuclear physicsTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)Particle and Plasma PhysicsDouble beta decay0103 physical sciencesDark Matter and Double Beta Decay (experiments)Calibrationlcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclearCalibratge010306 general physicsNuclear ExperimentMathematical PhysicsPhysicsQuantum Physics010308 nuclear & particles physicsDetectorMolecularDetectorsInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsCalibrationPhysical Scienceslcsh:QC770-798High Energy Physics::ExperimentSensitivity (electronics)Event (particle physics)Energy (signal processing)
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