Search results for " high energy physics"

showing 10 items of 8412 documents

Assessment of the importance of neutron multiplication for tritium production

2016

Abstract One of the major requirements for a fusion power plant in the future is tritium self-sufficiency. For this reason the scientific community has dedicated a lot of effort to research activity on reactor tritium breeding blankets. In the framework of the international project DEMO, many concepts of breeding blanket have been taken into account and some of them will be tested in the experimental reactor ITER by means of appropriate test blanket modules (TBMs). All the breeding blanket concepts rely on the adoption of binary systems composed of a material acting as neutronic multiplier and another as a breeder. This paper addresses a neutronic feature of these kinds of systems. In parti…

tritium breeding blanket neutronicsNuclear and High Energy PhysicsComputer scienceNuclear engineeringBlanketFusion powerCondensed Matter Physics01 natural sciences010305 fluids & plasmasNuclear physics0103 physical sciencesModel setNeutron multiplicationNeutronTritium010306 general physicsSettore ING-IND/19 - Impianti NucleariNuclear Fusion
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Erosion, screening, and migration of tungsten in the JET divertor

2019

The erosion of tungsten (W), induced by the bombardment of plasma and impurity particles, determines the lifetime of plasma-facing components as well as impacting on plasma performance by the influx of W into the confined region. The screening of W by the divertor and the transport of W in the plasma determines largely the W content in the plasma core, but the W source strength itself has a vital impact on this process. The JET tokamak experiment provides access to a large set of W erosion-determining parameters and permits a detailed description of the W source in the divertor closest to the ITER one: (i) effective sputtering yields and fluxes as function of impact energy of intrinsic (Be,…

tungsten divertorNuclear and High Energy PhysicsMaterials scienceNuclear engineeringchemistry.chemical_elementTungsten01 natural sciences010305 fluids & plasmaserosion and depositionASDEX UpgradePhysics::Plasma PhysicsImpurity0103 physical sciencesITER divertor010306 general physicsW spectroscopyJet (fluid)DivertorPlasmaequipment and suppliesCondensed Matter::Mesoscopic Systems and Quantum Hall EffectCondensed Matter PhysicsERO modellingchemistryJETPhysics::Space PhysicsErosionPhysics::Accelerator PhysicsAstrophysics::Earth and Planetary Astrophysicsddc:620Nuclear Fusion
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The OLYMPUS Experiment

2014

Nuclear instruments & methods in physics research / A 741, 1 - 17 (2014). doi:10.1016/j.nima.2013.12.035

two-photon [exchange]Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsHadronluminosity: monitoringRecoil4-MOMENTUM TRANSFERSNuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationNuclear ExperimentPhysicsElastic scatteringLuminosity (scattering theory)ELECTROMAGNETIC FORM-FACTORSInstrumentation and Detectors (physics.ins-det)elastic scattering [cross section]positron p: elastic scatteringAntimatterdrift chamberelastic scattering [electron p]target [hydrogen]proportional chamberCROSS-SECTIONNuclear and High Energy PhysicsELECTRON-PROTONDESY DORIS StorFOS: Physical sciencesmonitoring [luminosity]time-of-flight530electron p: elastic scatteringNuclear physicsCross section (physics)RATIO(GEV/C)(2)p: form factor: ratiocalorimeterddc:530cross section: elastic scatteringactivity reporthydrogen: targetexchange: two-photonScatteringPOSITRONSDESYelastic scattering [positron p]magnetic spectrometerELECTROMAGNETIC FORM-FACTORS; PROTON ELASTIC-SCATTERING; 4-MOMENTUM TRANSFERS; ELECTRON-PROTON; CROSS-SECTION; RATIO; (GEV/C)(2); POSITRONSform factor: ratio [p]gas electron multiplierPhysics::Accelerator PhysicsPROTON ELASTIC-SCATTERINGHigh Energy Physics::Experiment
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Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

2017

A search for ultra-high energy photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation mode. An unprecedented separation power between photon and hadron primaries is achieved by combining measurements of the longitudinal air-shower development with the particle content at ground measured by the fluorescence and surface detectors, respectively. Only three photon candidates at energies 1-2 EeV are found, which is compatible with the expected hadron-induced background. Upper limits on the integral flux of ultra-high energy photons of 0.027, 0.009, 0.008, 0.008 and 0.007 km-2 sr-1 yr-1 are derived at 95% C.L. for ener…

ultra high energy cosmic rays cosmic ray experimentsPhoton[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyHadronFluxultra high energy cosmic rays; cosmic ray experiments7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)energy: thresholdCosmic ray experiments[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsphoton: productionconstraint: energyCOSMIC-RAYSAugerobservatoryContent (measure theory)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenalongitudinalAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayultra high energy cosmic raysdark matterUltra high energy cosmic rays Cosmic ray experiments Astronomy and Astrophysics.Nuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesultra high energy cosmic rays; cosmic ray experiments; Astronomy and Astrophysicscosmic radiation: UHEHigh Energy PhysicsCiencias ExactasPierre Auger ObservatorySPECTRUMhybridbackgrounddetector: surface010308 nuclear & particles physicsFísicaUltra high energy cosmic raysAstronomy and AstrophysicsASTROFÍSICAULTRA-HIGH ENERGYfluxExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experimentshadron[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Ultra-High Energy Neutrinos at the Pierre Auger Observatory

2013

The observation of ultrahigh energy neutrinos (UHE nu s) has become a priority in experimental astroparticle physics. UHE nu s can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going nu) or in the Earth crust (Earth-skimming nu), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and …

ultra high energy neutrino[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsCiencias FísicasAstronomyFluxAstrophysics7. Clean energy01 natural sciencesAltas energíasAuger//purl.org/becyt/ford/1 [https]surface [detector]ObservatoryneutriniCosmic-rayscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCascada atmosférica extensaOBSERVATÓRIOS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsneutrino; Augerlcsh:QC1-999AugercascadeUHE [neutrino]observatoryPhysics::Space PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearultra high energy neutrinosNeutrinoAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASsignatureTAU-NEUTRINOSatmosphere [showers]FLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Article SubjectairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayFísica de Partículas y CamposLIMITPartícules (Física nuclear)Ultra high energy cosmic rayAtmosphere[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Air-showersSEARCHNeutrino0103 physical sciencesddc:530010306 general physicsAstrophysiqueCiencias ExactasPierre Auger ObservatoryAstroparticle physicsSPECTRUM010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaUltra high energy cosmic raystelescopes//purl.org/becyt/ford/1.3 [https]Ultrahigh Energyflux13. Climate actionenergy [neutrino]Pierre AugerExperimental High Energy PhysicsARRAYHigh Energy Physics::ExperimentAstroparticle physicslcsh:Physics
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Measurement of dielectron production in central Pb-Pb collisions at √sNN = 2.76 TeV

2019

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. The first measurement of dielectron (e + e −) production in central (0 – 10 %) Pb – Pb collisions at √sNN=2.76TeV at the LHC is presented. The dielectron invariant-mass spectrum is compared to the expected contributions from hadron decays in the invariant-mass range 0 < mee < 3.5 GeV / c2. The ratio of data and the cocktail of hadronic contributions without vacuum ρ0 is measured in the invariant-mass range 0.15 < mee < 0.7 GeV / c2, w…

virtual [photon]:Kjerne- og elementærpartikkelfysikk: 431 [VDP]heavy ion collisionsHadrondielectron productionhiukkasfysiikkaPP01 natural sciencesS-W INTERACTIONSthermalALICEPhysics::Atomic PhysicsNuclear ExperimentBrookhaven RHIC CollPhysicsAU COLLISIONSLarge Hadron Colliderphoton: virtual ; photon: direct production ; heavy ion: scattering ; hadron: decay ; Brookhaven RHIC Coll ; transverse momentum ; CERN LHC Coll ; thermal ; ALICE ; mesonVDP::Kjerne- og elementærpartikkelfysikk: 431DIRECT PHOTON PRODUCTIONddc::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]PRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]CERN LHC CollVDP::Nuclear and elementary particle physics: 431Transverse momentumNuclear and High Energy PhysicsRho mesondirect production [photon]MesonPAIR PRODUCTIONPhoton lepton & quark productiontransverse momentumFew-body systemsmesonNuclear physicsDIRECT PHOTON PRODUCTION; S-W INTERACTIONS; AU COLLISIONS; RHO-MESON; DIMUON PRODUCTION; PAIR PRODUCTION; PP; J/PSI; ENHANCEMENT; EMISSIONENHANCEMENTscattering [heavy ion]0103 physical sciencesRelativistic heavy-ion collisionsRHO-MESON010306 general physicsParticle & resonance productionNuclear Physicsta114010308 nuclear & particles physics:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]NATURAL SCIENCES. Physics.J/PSIPair productionDIMUON PRODUCTIONQuark–gluon plasmaHigh Energy Physics::ExperimentEMISSIONdecay [hadron]
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Search for inelastic scattering of WIMP dark matter in XENON1T

2021

We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off $^{129}$Xe is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV de-excitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.89 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2$\sigma$. A profile-likelihood ratio analysis is used to set upper limits on the cross-section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c${}^2$, with the strongest upper limit of $3.3 \time…

xenon: targetPhotonPhysics::Instrumentation and DetectorsParameter space01 natural sciencesWIMP: dark matterHigh Energy Physics - Experiment; High Energy Physics - Experiment; astro-ph.COHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XENONRecoilWIMPWIMP nucleus: cross section[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterparameter spaceNuclear ExperimentComputingMilieux_MISCELLANEOUSnucleus: recoilPhysicsDark Matter Inelastic scattering XENON Direct Dark MatterPhysicsphotonAstrophysics::Instrumentation and Methods for AstrophysicsDirect Dark MatterWeakly interacting massive particlesastro-ph.COsignatureAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsInelastic scatteringCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesWIMP: massAstrophysics::Cosmology and Extragalactic AstrophysicsInelastic scatteringNOPE2_2PE2_10103 physical sciencesddc:530010306 general physics010308 nuclear & particles physicsScatteringWIMP nucleus: interactionDarkmatterWIMP: interactionHigh Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physicsexperimental resultsPhysical Review D. Particles, Fields, Gravitation, and Cosmology
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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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Evidence against the wobbling nature of low-spin bands in 135Pr

2021

International audience; The electromagnetic character of the ΔI=1 transitions connecting the 1- to 0-phonon and the 2- to 1-phonon wobbling bands should be dominated by an E2 component, due to the collective motion of the entire nuclear charge. In the present work it is shown, based on combined angular correlation and linear polarization measurements, that the mixing ratios of all analyzed connecting transitions between low-lying bands in 135Pr interpreted as 0-, 1-, and 2-phonon wobbling bands, have absolute values smaller than one. This indicates predominant M1 magnetic character, which is incompatible with the proposed wobbling nature. All experimental observables are instead in good agr…

γγγ-coincidencesNuclear and High Energy Physics010308 nuclear & particles physicsPhysicsQC1-999FOS: Physical sciences-coincidences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex01 natural sciencesParticle rotor modelAngular correlationsspin (kvanttimekaniikka)0103 physical sciencesWobbling bandsNuclear Physics - ExperimentNuclear Experiment (nucl-ex)ydinfysiikka010306 general physicsNuclear Experiment
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Search for scalar leptoquarks in pp collisions at $\sqrt{s}$=13 TeV with the ATLAS experiment

2016

An inclusive search for a new-physics signature of lepton-jet resonances has been performed by the ATLAS experiment. Scalar leptoquarks, pair-produced in pp collisions at s √s = 13 TeV at the large hadron collider, have been considered. An integrated luminosity of 3.2 fb-1, corresponding to the full 2015 dataset was used. First (second) generation leptoquarks were sought in events with two electrons (muons) and two or more jets. The observed event yield in each channel is consistent with Standard Model background expectations. The observed (expected) lower limits on the leptoquark mass at 95% confidence level are 1100 and 1050 GeV (1160 and 1040 GeV) for first and second generation leptoqua…

Большой адронный коллайдер13000 GeV-cms((n)jet dilepton) [final state]General Physics and AstronomyElementary particleleptoquark7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)Subatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]leptoquark; ATLAS; LHC; PARTON DISTRIBUTIONS; LHCлептокваркипротон-протонные столкновенияQCPhysicsLarge Hadron Colliderleptoquark --> quark leptonATLAS experimentSettore FIS/01 - Fisica SperimentaleATLASmass dependencebranching ratio [leptoquark]CERN LHC Collleptoquark ATLAS LHCLHCcolliding beams [p p]Particle Physics - ExperimentQuarkParticle physicsleptoquark --> quark neutrino530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]signature [new physics]leptoquark; ATLAS; LHCFOS: Physical sciencesLHC ATLAS High Energy Physicsddc:500.2530Nuclear physicsPhysics and Astronomy (all)510 Mathematicsscalar [leptoquark]0103 physical sciencesLeptoquarkddc:530High Energy Physics010306 general physicsCiencias Exactasupper limit [mass]MuonScience & Technologyhep-ex010308 nuclear & particles physicsBranching fractionbackgroundATLAS; Leptoquark; LHC; High Energy Physics - Experiment; High Energy Physics - Experiment; Physics and Astronomy (all)High Energy Physics::PhenomenologyFísicasensitivitymass [leptoquark]PARTON DISTRIBUTIONSLeptoquarkExperimental High Energy Physicsupper limit [branching ratio]High Energy Physics::ExperimentATLAS детекторATLAS; Leptoquark; LHC; Physics and Astronomy (all)Leptonexperimental results
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