Search results for " high energy physics"

showing 10 items of 8412 documents

Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

2019

Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming τ neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in ∼ 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an Eν -2 spectrum in the energy range 1.0 × 1017 eV -2.5 × 1019 eV is E2 dNν/dEν < 4.4 × 10-9 GeV cm-2 s-1 sr-1, placing str…

cosmological neutrinosAstronomyFluxAstrophysics01 natural sciences7. Clean energycosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic rayssurface [detector]Ultra-high-energy cosmic rayPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)cosmological neutrinoSettore FIS/01 - Fisica SperimentaleDETETORESneutrino: UHEUHE [neutrino]Augerobservatorytrajectoryneutrino: flavorProduction (computer science)NeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencescosmic ray experimentCosmic rayultra high energy cosmic raysneutrino: productionneutrino astronomyproduction [neutrino]TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530model [neutrino]High Energy Physicscosmic radiation: UHEZenithAstrophysiqueneutrino: modelPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsdetector: surfaceHigh Energy Physics::Phenomenologyflavor [neutrino]Astronomy and AstrophysicsAstronomiefluxExperimental High Energy PhysicsatmosphereHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

2019

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60 in declination, with peak sensitivities at declinations around ∼-53 and ∼+55, and an unmatched sensitivity for arrival directions in the Northern hemisphere. A search has been performed for highly-inclined air showers induced by neutrinos of all flavours with no candidate events found in data taken between 1 Jan 2004 and 31 Aug 2018. Upper limits on the neutrino flux from point-like steady sources have been derived as a function of source declination. An unrivaled sensit…

cosmological neutrinosAstronomypoleFluxAstrophysics01 natural sciencesneutrino: fluxcosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic raysmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSastro-ph.HEcosmological neutrinoSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSneutrino: UHEAugerobservatoryNEUTRINOSNeutrinoAstrophysics - High Energy Astrophysical Phenomenaairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesultra high energy cosmic raysDeclinationneutrino astronomyCelestial pole0103 physical sciencesflux: upper limitHigh Energy PhysicsDETECTORZenithAstrophysiquePierre Auger Observatoryflavorshowers: atmosphere010308 nuclear & particles physicsdetector: surfaceNorthern HemisphereAstronomy and AstrophysicsAstronomiesensitivitySkyExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Measurements of inclusive jet spectra in pp and central Pb-Pb collisions at √sNN = 5.02 TeV

2020

This article reports measurements of the pT-differential inclusive jet cross section in pp collisions at √s = 5.02 TeV and the pT-differential inclusive jet yield in Pb-Pb 0-10% central collisions at √sNN = 5.02 TeV. Jets were reconstructed at midrapidity with the ALICE tracking detectors and electromagnetic calorimeter using the anti-kT algorithm. For pp collisions, we report jet cross sections for jet resolution parameters R=0.1-0.6 over the range 20<pT,jet<140 GeV/c, as well as the jet cross-section ratios of different R and comparisons to two next-to-leading-order (NLO)-based theoretical predictions. For Pb-Pb collisions, we report the R=0.2 and R=0.4 jet spectra for 40<pT,jet<140 GeV/c…

cross-sectionNuclear and High Energy Physicshotquark-gluon plasmaAstrophysics::High Energy Astrophysical PhenomenaperspectiveHigh Energy Physics::ExperimentdependencesuppressionhiukkasfysiikkaNuclear Experimentradiusmatter
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Estimating QCD uncertainties in Monte Carlo event generators for gamma-ray dark matter searches

2018

Motivated by the recent galactic center gamma-ray excess identified in the Fermi-LAT data, we perform a detailed study of QCD fragmentation uncertainties in the modeling of the energy spectra of gamma-rays from Dark-Matter (DM) annihilation. When Dark-Matter particles annihilate to coloured final states, either directly or via decays such as $W^{(*)}\to q\bar{q}'$, photons are produced from a complex sequence of shower, hadronisation and hadron decays. In phenomenological studies, their energy spectra are typically computed using Monte Carlo event generators. These results have however intrinsic uncertainties due to the specific model used and the choice of model parameters, which are diffi…

dark matter simulationsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonAstrophysics::High Energy Astrophysical Phenomenamodel [hadronization]SLDgamma ray theoryDark matterMonte Carlo methodHadronFOS: Physical sciencesmass [dark matter]01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)fragmentationquantum chromodynamics0103 physical sciencesconservation lawddc:530High Energy PhysicsMonte Carloenergy spectrum [gamma ray]Quantum chromodynamicsPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsphotonGamma rayCERN LEP StorAstronomy and AstrophysicsshowersGalaxyHigh Energy Physics - PhenomenologyannihilationExperimental High Energy PhysicsHigh Energy Physics::Experimentgalaxydecay [hadron]GLAST [interpretation of experiments]Astrophysics - 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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Measurement of θ13 in Double Chooz using neutron captures on hydrogen with novel background rejection techniques

2016

The Double Chooz collaboration presents a measurement of the neutrino mixing angle θ[subscript 13] using reactor [bar over ν[subscript e]] observed via the inverse beta decay reaction in which the neutron is captured on hydrogen. This measurement is based on 462.72 live days data, approximately twice as much data as in the previous such analysis, collected with a detector positioned at an average distance of 1050 m from two reactor cores. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties. Accidental coincidences, the dominant background in this analysis, are suppressed by more than an order of magnitude with respec…

data analysis methodNuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsNeutrino Detectors and TelescopeGadoliniumnuclear reactor [antineutrino/e]energy spectrumchemistry.chemical_elementFluxmixing angle: measured [neutrino]CHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - Experimentflux [antineutrino]Flavor physicscapture [n]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interactionddc:530Neutron010306 general physicsPhysicsNeutrino Detectors and Telescopesbackground010308 nuclear & particles physicsoscillation [neutrino]suppressionDouble ChoozNeutron captureOscillationchemistryhydrogenInverse beta decayFlavor physicspectralHigh Energy Physics::ExperimentgadoliniumNeutrinoOrder of magnitudeexperimental results
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Resolution Characterizations of JetRIS in Mainz Using 164Dy

2022

Atoms 10(2), 57 (2022). doi:10.3390/atoms10020057

de Laval nozzlenobeliumNuclear and High Energy PhysicsScience & TechnologyRESONANCE IONIZATION SPECTROSCOPYPhysicsJetRIS; fluorescence spectroscopy; gas-jet; de Laval nozzle; nobeliumPhysics Atomic Molecular & Chemicalfluorescence spectroscopyCondensed Matter Physics530Atomic and Molecular Physics and OpticsJetRISPhysical SciencesELEMENTSgas-jetddc:530Physics::Atomic PhysicsNuclear ExperimentLASER SPECTROSCOPYAtoms
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Measurements of the top quark branching ratios into channels with leptons and quarks with the ATLAS detector

2015

Measurements of the branching ratios of top quark decays into leptons and jets using events with t[bar over t] (top antitop) pairs are reported. Events were recorded with the ATLAS detector at the LHC in pp collisions at a center-of-mass energy of 7 TeV. The collected data sample corresponds to an integrated luminosity of 4.6  fb[superscript −1]. The measured top quark branching ratios agree with the Standard Model predictions within the measurement uncertainties of a few percent.

decay [top]Top quarkБольшой адронный коллайдерAtlas detectormeasured [cross section]верхние кваркиpair production [top]multiplicity [lepton]High Energy Physics - ExperimentScatteringSubatomär fysikHigh Energy Physics - Experiment (hep-ex)лептоныSubatomic PhysicsJets[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]CollisionsSUPERSYMMETRYGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)протон-протонные столкновенияQCPhysicsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleSupersymmetryATLASTop Quark Branching RatiosCERN LHC CollProton–proton collisions7000 GeV-cmsPAIR CROSS-SECTIONcolliding beams [p p]Particle Physics - Experiment((n)jet lepton) [final state]top quark branching ratios; leptons; quarks; ATLAS detectorQuarkParticle physicsNuclear and High Energy PhysicsCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesPAIR CROSS-SECTION; PARTON DISTRIBUTIONS; PP COLLISIONS; SUPERSYMMETRY; TEVBranching (polymer chemistry)Accelerator Physics and Instrumentation530Nuclear physicsddc:530Science & TechnologyPP COLLISIONSScatteringHigh Energy Physics::PhenomenologyFísicaAcceleratorfysik och instrumenteringLeptons and Quarksbranching ratio: measured [top]PARTON DISTRIBUTIONSExperimental High Energy PhysicsTEVp p --> 2top anythingHigh Energy Physics::ExperimentATLAS детекторhadronic decay [tau]Leptonexperimental results
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Performance of $b$-Jet Identification in the ATLAS Experiment

2016

We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT an…

detector-systems performancePerformance of High Energy Physics Detectorsecondary [vertex]Elementary particle01 natural sciencesPARTONlaw.inventionSubatomär fysikCHANNELcluster findingscattering [p p]impact parameterGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)протон-протонные столкновенияQBLarge detector-systems performanceHigh energy physics detectorLarge Hadron ColliderLarge detector systems for particle and astroparticle physics; Large detector-systems performance; Pattern recognition cluster finding calibration and fitting methods; Performance of High Energy Physics Detectors; Instrumentation; Mathematical Physicstrack data analysisQUARK PAIR PRODUCTIONbottom [jet]CERN LHC CollPattern recognition cluster finding calibration and fitting method7000 GeV-cmscolliding beams [p p]performanceHADRONIC COLLISIONSCiências Naturais::Ciências FísicasLarge detectorFitting methodHigh energy physicATLAS LHC High Energy Physics510 MathematicsmuonDISTRIBUTIONSUncertainty analysis Astroparticle physicHigh Energy Physics010306 general physicsSystematic uncertainties AlgorithmsAstroparticle physicsCalibration and fitting methodsScience & Technology010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsParticle acceleratorRangingPerformance of High Energy PhysicsCOLLIDERScorrelationExperimental High Energy PhysicsPerformance of High Energy Physics DetectorshadronATLAS детекторБольшой адронный коллайдерcharm [jet]Elementary particleHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesInstrumentationUncertainty analysisMathematical PhysicsPhysicsPattern recognition cluster finding calibration and fitting methods4. EducationATLAS experimentSettore FIS/01 - Fisica SperimentaleDetectorsflavor [jet]calibration and fitting methodsATLASLarge Hadron ColliderLarge detector systems for particle and astroparticle physics; Large; detector-systems performance; Pattern recognition cluster finding; calibration and fitting methods; Performance of High Energy Physics; Detectors; PRODUCTION CROSS-SECTION; QUARK PAIR PRODUCTION; ROOT-S=7 TEV; PARTON; DISTRIBUTIONS; HADRONIC COLLISIONS; MATRIX-ELEMENTS; LHC; COLLIDERS; DETECTOR; CHANNEL8. Economic growthCalibrationparticle identification [bottom]LHCImpact parameterParticle Physics - ExperimentParticle physicsdata analysis method530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciences530MATRIX-ELEMENTSparticle identification [charm]on-line [trigger]Pattern recognition0103 physical sciencesComplementary methodddc:610DETECTORROOT-S=7 TEVCluster findingFísicaLarge detector systems for particle and astroparticle physics; Large detector-systems performance; Pattern recognition cluster finding calibration and fitting methods; Performance of High Energy Physics DetectorsPattern recognition systemcalibrationtracksPRODUCTION CROSS-SECTIONefficiencyHadronLarge detector systems for particle and astroparticle physicLargeHigh Energy Physics::ExperimentStatistical correlationstatisticalexperimental results
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Measurement of the spin-dependent structure function g1(x) of the deuteron

1993

We report on the first measurement of the spin-dependent structure function g1d of the deuteron in the deep inelastic scattering of polarised muons off polarised deuterons, in the kinematical range 0.006&lt;x&lt;0.6, 1 GeV2&lt;Q2&lt;30 GeV2. The first moment, Γ1d=sh{phonetic}01 g1d dx=0.023±0.020 (stat.) ± 0.015 (syst.), is smaller than the prediction of the Ellis-Jaffe sum rules. Using earlier measurements of g1p, we infer the first moment of the spin-dependent neutron structure function g1n. The difference Γ1p-Γ1n=0.20 ±0.05 (stat.) ± 0.04 (syst.) agrees with the prediction of the Bjorken sum rule, Γ1p-Γ1n=0.191 ±0.002.

deuteron: polarized targetNuclear and High Energy PhysicsINELASTIC E-P; POLARIZED PROTONS; SUM-RULE; SCATTERING; ELECTROPRODUCTION; ASYMMETRYINELASTIC E-PProtonpolarized target: deuterondeep inelastic scattering: muon deuteronstructure function: spinmuon deuteron: deep inelastic scatteringSUM-RULE530Nuclear physicsINELASTIC E-P; POLARIZED PROTONS; SUM-RULE; SCATTERING; ELECTROPRODUCTION; ASYMMETRY; MODELTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYSCATTERINGNeutronpolarized beam: muonSpin-½PhysicsQuantum chromodynamicsspin: structure functionMuonScatteringdeuteron: structure functionELECTROPRODUCTIONnucleon: structure functionCERN SPSDeep inelastic scatteringmomentmagnetic spectrometer: experimental resultsPOLARIZED PROTONSapprox. 100 GeVASYMMETRYSum rule in quantum mechanicsmuon: polarized beamParticle Physics - ExperimentPhysics Letters B
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