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showing 10 items of 3080 documents

Evidence of Electron Neutrino Appearance in a Muon Neutrino Beam

2013

The T2K Collaboration reports evidence for electron neutrino appearance at the atmospheric mass splitting, vertical bar Delta m(32)(2)vertical bar approximate to 2.4 X 10(-3) eV(2). An excess of electron neutrino interactions over background is observed from a muon neutrino beam with a peak energy of 0.6 GeV at the Super-Kamiokande (SK) detector 295 km from the beam's origin. Signal and background predictions are constrained by data from near detectors located 280 m from the neutrino production target. We observe 11 electron neutrino candidate events at the SK detector when a background of 3.3 +/- 0.4(syst) events is expected. The background-only hypothesis is rejected with a p value of 0.0…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciencesFluxddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Pion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Momentum rangeMuon neutrino010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsT2K experimentFísicaHigh Energy Physics::ExperimentNeutrinoAbsorption cross-sectionsElectron neutrinoBeam (structure)
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An improved method for measuring muon energy using the truncated mean of dE/dx

2012

Nuclear instruments & methods in physics research / A 703, 190 - 198 (2013). doi:10.1016/j.nima.2012.11.081

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciencesddc:500.2Cherenkov; dE/dx; IceCube detector; Muon energy; Neutrino energy; Truncated mean53001 natural sciencesParticle detectorParticle identificationNuclear physicsdE/dx0103 physical sciencesSpecific energyddc:530CherenkovNeutrino energyInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonTruncated meanMuon energy010308 nuclear & particles physicsDE/dxPhysics - Data Analysis Statistics and ProbabilityScintillation counterHigh Energy Physics::ExperimentNeutrinoIceCube detectorAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsData Analysis Statistics and Probability (physics.data-an)Lepton
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Measurement of the Z→ττ cross section with the ATLAS detector

2011

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsHadronElementary particleddc:500.25307. Clean energy01 natural sciencesPartícules (Física nuclear)Nuclear physics0103 physical sciencesNuclear Experiment010306 general physicsQCPhysicsLarge Hadron ColliderMuon010308 nuclear & particles physicsBranching fractionAtlas (topology)High Energy Physics::PhenomenologyATLAS experimentFísicacross section; leptonsFísica nuclearHigh Energy Physics::ExperimentLepton
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Measurement of the atmospheric neutrino energy spectrum from 100 GeV to 400 TeV with IceCube

2010

A measurement of the atmospheric muon neutrino energy spectrum from 100 GeV to 400 TeV was performed using a data sample of about 18,000 up-going atmospheric muon neutrino events in IceCube. Boosted decision trees were used for event selection to reject mis-reconstructed atmospheric muons and obtain a sample of up-going muon neutrino events. Background contamination in the final event sample is less than one percent. This is the first measurement of atmospheric neutrinos up to 400 TeV, and is fundamental to understanding the impact of this neutrino background on astrophysical neutrino observations with IceCube. The measured spectrum is consistent with predictions for the atmospheric muon ne…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesDeep IceSouth-PoleHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)ddc:530Muon neutrinoNeutrino oscillationPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)FluxHigh Energy Physics::PhenomenologyOptical-PropertiesDetectorSolar neutrino problemHigh Energy Physics - PhenomenologyNeutrino detectorMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaTelescopesPhys.Rev.D
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T2K neutrino flux prediction

2013

The Tokai-to-Kamioka (T2K) experiment studies neutrino oscillations using an off-axismuon neutrino beam with a peak energy of about 0.6 GeV that originates at the Japan Proton Accelerator Research Complex accelerator facility. Interactions of the neutrinos are observed at near detectors placed at 280 m from the production target and at the far detector-Super-Kamiokande-located 295 km away. The flux prediction is an essential part of the successful prediction of neutrino interaction rates at the T2K detectors and is an important input to T2K neutrino oscillation and cross section measurements. A FLUKA and GEANT3-based simulation models the physical processes involved in the neutrino producti…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaddc:500.2Antiprotons01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsPions0103 physical sciencesMomentum rangeMuon neutrino010306 general physicsNeutrino oscillationNuclear ExperimentQCPhysicsGev-c010308 nuclear & particles physicsParticle-productionHigh Energy Physics::PhenomenologyT2K experimentFísicaDetectorMonitorSolar neutrino problemNucleiNeutrino detector13. Climate actionMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoProtonsAbsorption cross-sectionsParticle Physics - Experiment
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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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Search for stable hadronising squarks and gluinos with the ATLAS experiment at the LHC

2011

Hitherto unobserved long-lived massive particles with electric and/or colour charge are predicted by a range of theories which extend the Standard Model. In this Letter a search is performed at the ATLAS experiment for slow-moving charged particles produced in proton–proton collisions at 7 TeV centre-of-mass energy at the LHC, using a data-set corresponding to an integrated luminosity of 34 pb[superscript −1]. No deviations from Standard Model expectations are found. This result is interpreted in a framework of supersymmetry models in which coloured sparticles can hadronise into long-lived bound hadronic states, termed R-hadrons, and 95% CL limits are set on the production cross-sections of…

Nuclear and High Energy PhysicsParticle physicsR-hadronCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]HadronATLAS experimentFOS: Physical sciencesddc:500.253001 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Supersymmetry; Long-lived particle; R-hadron; LimitMASSIVE CHARGED PARTICLES0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fysikddc:530High Energy Physics010306 general physicsPhysicsGluinoLarge Hadron ColliderScience & Technology010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleATLAS experimentHigh Energy Physics::PhenomenologyFísicaSuperpartnerSupersymmetryATLASLong-lived particleCharged particleR-hadronPhysical SciencesExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentLHCSupersymmetryLimitlimit; supersymmetry; long-lived particle; r-hadronParticle Physics - Experiment
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The radiative decay of the Lambda(1405) and its two-pole structure

2007

We evaluate theoretically the radiative decay widths into $\gamma\Lambda$ and $\gamma\Sigma^0$ of the two poles of the $\Lambda(1405)$ found in chiral unitary theories and we find quite different results for each of the two poles. We show that, depending on which reaction is used to measure the $\Lambda(1405)$ radiative decays, one gives more weight to one or the other pole, resulting in quite different shapes in the $\gamma\Lambda(\Sigma^0)$ invariant mass distributions. Our results for the high-energy pole agree with those of the empirical determination of the $\gamma\Lambda$ and $\gamma\Sigma^0$ radiative widths (based on an isobar model fitting of the $K^-p$ atom data), which are someti…

Nuclear and High Energy PhysicsParticle physicsRadiative decayStructure (category theory)radiative decay [Lambda(1405)]chiral [perturbation theory]Lambda(Sigma0 photon) [mass spectrum]Measure (mathematics)Lambda(1405) --> Lambda photonK- p --> Lambda pi0 photonK- p --> Sigma0 pi0 photonAtompi- p --> Lambda K0 photonpi- p --> Sigma0 K0 photonRadiative transferddc:530Invariant massnumerical calculationsPhysicsLambda(1405) --> Sigma0 photonSigma0inelastic scattering [K- p]Físicapole [approximation]hadroproduction [Lambda(1405)]High Energy Physics - Phenomenology(Lambda photon) [mass spectrum]Isobarinelastic scattering [pi- p]hadroproduction [hyperon]width [Lambda(1405)]
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Status of Light Sterile Neutrino Searches

2020

A number of anomalous results in short-baseline oscillation may hint at the existence of one or more light sterile neutrino states in the eV mass range and have triggered a wave of new experimental efforts to search for a definite signature of oscillations between active and sterile neutrino states. The present paper aims to provide a comprehensive review on the status of light sterile neutrino searches in mid-2019: we discuss not only the basic experimental approaches and sensitivities of reactor, source, atmospheric, and accelerator neutrino oscillation experiments but also the complementary bounds arising from direct neutrino mass experiments and cosmological observations. Moreover, we r…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBibliographyddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsOscillationHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Cosmological modelHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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The T2K Experiment

2011

The T2K experiment is a long-baseline neutrino oscillation experiment. Its main goal is to measure the last unknown lepton sector mixing angle {\theta}_{13} by observing {\nu}_e appearance in a {\nu}_{\mu} beam. It also aims to make a precision measurement of the known oscillation parameters, {\Delta}m^{2}_{23} and sin^{2} 2{\theta}_{23}, via {\nu}_{\mu} disappearance studies. Other goals of the experiment include various neutrino cross section measurements and sterile neutrino searches. The experiment uses an intense proton beam generated by the J-PARC accelerator in Tokai, Japan, and is composed of a neutrino beamline, a near detector complex (ND280), and a far detector (Super-Kamiokande)…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and Detectorsddc:500.27. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Long baseline[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinos010306 general physicsNeutrino oscillationphysics.ins-detInstrumentationQCPhysicsT2Khep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyT2K experimentNeutrinos; Neutrino oscillation; Long baseline; T2K; J-PARC; Super-KamiokandeFísicaNeutrino detectorJ-PARCHigh Energy Physics::ExperimentJ-PARCSuper-KamiokandeNeutrinoSuper-KamiokandeLepton
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