Search results for "high-energy"

showing 10 items of 161 documents

Total-scattering pair-distribution function of organic material from powder electron diffraction data.

2014

AbstractThis paper shows that pair-distribution function (PDF) analyses can be carried out on organic and organometallic compounds from powder electron diffraction data. Different experimental setups are demonstrated, including selected area electron diffraction and nanodiffraction in transmission electron microscopy or nanodiffraction in scanning transmission electron microscopy modes. The methods were demonstrated on organometallic complexes (chlorinated and unchlorinated copper phthalocyanine) and on purely organic compounds (quinacridone). The PDF curves from powder electron diffraction data, called ePDF, are in good agreement with PDF curves determined from X-ray powder data demonstrat…

Materials scienceReflection high-energy electron diffractionElectron diffractionGas electron diffractionScanning transmission electron microscopyAnalytical chemistryEnergy filtered transmission electron microscopySelected area diffractionInstrumentationPowder diffractionElectron backscatter diffractionMicroscopy and microanalysis : the official journal of Microscopy Society of America, Microbeam Analysis Society, Microscopical Society of Canada
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Structure characterization of hard materials by precession electron diffraction and automatic diffraction tomography: 6H-SiC semiconductor and Ni1+xT…

2012

Using a combination of automated diffraction tomography and precession electron diffraction techniques, quasi-kinematical electron diffraction data sets were collected from intermetallic Ni1+xTe1 embedded nanodomains and ion-thinned specimens of 6H–SiC semiconductor. Cell parameters and space groups were found automatically from the reconstructed 3D diffraction volume. The extracted intensities were used for fast ab initio structure determination by direct methods.

Materials scienceReflection high-energy electron diffractionGas electron diffractionbusiness.industryPhysics::OpticsCondensed Matter PhysicsMolecular physicsElectronic Optical and Magnetic MaterialsDiffraction tomographyCondensed Matter::Materials ScienceOpticsElectron diffractionMaterials ChemistryPrecession electron diffractionElectrical and Electronic EngineeringSelected area diffractionbusinessPowder diffractionElectron backscatter diffraction
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Structure analysis of side chain liquid crystal polymer films by means of electron microscopy

1987

Abstract Using the combined techniques of electron diffraction, bright and dark field electron microscopy as well as light microscopy, it has been possible to obtain detailed structural information about the arrangement of the smectic layers in a polymethacrylate side chain liquid crystal polymer with a biphenylester as the mesogenic group.

Materials scienceReflection high-energy electron diffractionbusiness.industryPolymer characterizationCryo-electron microscopyGeneral ChemistryCondensed Matter PhysicsDark field microscopyCondensed Matter::Soft Condensed MatterCrystallographyOpticsElectron diffractionLiquid crystalSide chainEnergy filtered transmission electron microscopyGeneral Materials SciencebusinessLiquid Crystals
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CERN-MEDICIS: A Review Since Commissioning in 2017

2021

The CERN-MEDICIS (MEDical Isotopes Collected from ISolde) facility has delivered its first radioactive ion beam at CERN (Switzerland) in December 2017 to support the research and development in nuclear medicine using non-conventional radionuclides. Since then, fourteen institutes, including CERN, have joined the collaboration to drive the scientific program of this unique installation and evaluate the needs of the community to improve the research in imaging, diagnostics, radiation therapy and personalized medicine. The facility has been built as an extension of the ISOLDE (Isotope Separator On Line DEvice) facility at CERN. Handling of open radioisotope sources is made possible thanks to i…

Medicine (General)HIGH-ENERGYIon beamNuclear engineeringHigh resolutionProton Synchrotron Booster01 natural sciencesmedicalISOLDE030218 nuclear medicine & medical imaginglaw.invention03 medical and health sciencesR5-9200302 clinical medicineMedicine General & InternallawGeneral & Internal Medicine0103 physical sciencesCERNNuclear Physics - ExperimentBeam dump010306 general physicsradionuclidesOriginal ResearchLarge Hadron ColliderScience & TechnologyGeneral MedicineMass separationHandling systemmass separationBeamlineMEDICISMedicineEnvironmental scienceLife Sciences & Biomedicine
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Swings between rotation and accretion power in a binary millisecond pulsar

2013

It is thought that neutron stars in low-mass binary systems can accrete matter and angular momentum from the companion star and be spun-up to millisecond rotational periods1, 2, 3. During the accretion stage, the system is called a low-mass X-ray binary, and bright X-ray emission is observed. When the rate of mass transfer decreases in the later evolutionary stages, these binaries host a radio millisecond pulsar4, 5 whose emission is powered by the neutron star’s rotating magnetic field6. This evolutionary model is supported by the detection of millisecond X-ray pulsations from several accreting neutron stars7, 8 and also by the evidence for a past accretion disc in a rotation-powered milli…

NEUTRON-STARSAstrophysics::High Energy Astrophysical PhenomenaBinary numberAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsBinary pulsarX-RAY TRANSIENTSRADIO PULSARSSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsarAstrophysics::Solar and Stellar AstrophysicsSAX J1808.4-3658Astrophysics::Galaxy AstrophysicsPhysicsMultidisciplinaryAstronomyHIDDENORBITCATALOGAccretion (astrophysics)EVOLUTIONNeutron starSPINHigh-energy astrophysicAstrophysics::Earth and Planetary AstrophysicsLow MassEMISSIONHigh-energy astrophysics; X-RAY TRANSIENTS; SAX J1808.4-3658; NEUTRON-STARS; RADIO PULSARS; EVOLUTION; EMISSION; SPIN; CATALOG; HIDDEN; ORBITX-ray pulsarNature
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Initial stages of self-assembled InAs/InP(001) quantum wire formation

2007

4 páginas, 2 figuras.-- PACS codes: 78.67.Lt; 68.65.La; 68.37.Ps.-- Comunicación oral presentada a la 14ª International Conference on Molecular Beam Epitaxy - MBE XIV celebrada en Tokio (Japón) del 3 al 8 de Septiembre de 2006.

NanostructureMaterials scienceReflection high-energy electron diffractionCondensed matter physicsQuantum wireA3. Molecular beam epitaxyRelaxation (NMR)NucleationB2. Semiconducting indium phosphideCondensed Matter PhysicsA1. NucleationInorganic ChemistryReflection (mathematics)Electron diffractionA1. NanostructuresMaterials ChemistryMolecular beam epitaxyJournal of Crystal Growth
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Deployment of the ATLAS High-Level Trigger

2006

The ATLAS combined test beam in the second half of 2004 saw the first deployment of the ATLAS High-Level Trigger (HLT). The next steps are deployment on the pre-series farms in the experimental area during 2005, commissioning and cosmics tests with the full detector in 2006 and collisions in 2007. This paper reviews the experience gained in the test beam, describes the current status and discusses the further enhancements to be made. We address issues related to the dataflow, integration of selection algorithms, testing, software distribution, installation and improvements.

Nuclear and High Energy PhysicsDataflowCluster (spacecraft)01 natural sciencesAtlas (anatomy)testbeam0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]medicineElectrical and Electronic EngineeringSelection algorithmSimulationhigh-level triggersPhysicshigh-energy physics010308 nuclear & particles physicsbusiness.industryDetectorATLASSoftware distributionTriggertriggeringmedicine.anatomical_structureNuclear Energy and EngineeringClustersoftware integrationSoftware deploymentSystems engineeringSystem integrationLHCbusinessIEEE Transactions on Nuclear Science
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Lateral distribution of muons in IceCube cosmic ray events

2013

In cosmic ray air showers, the muon lateral separation from the center of the shower is a measure of the transverse momentum that the muon parent acquired in the cosmic ray interaction. IceCube has observed cosmic ray interactions that produce muons laterally separated by up to 400 m from the shower core, a factor of 6 larger distance than previous measurements. These muons originate in high pT (>2  GeV/c) interactions from the incident cosmic ray, or high-energy secondary interactions. The separation distribution shows a transition to a power law at large values, indicating the presence of a hard pT component that can be described by perturbative quantum chromodynamics. However, the ra…

Nuclear and High Energy PhysicsENERGIESPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsddc:500.201 natural sciences7. Clean energyPower lawIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencescosmic radiation : interactionddc:530Charm (quantum number)Ultra-high-energy cosmic ray010306 general physicsZenithPhysicsQuantum chromodynamicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsGluonMODELPhysics and Astronomy13. Climate actionTEVHigh Energy Physics::ExperimentGLUONAstrophysics - High Energy Astrophysical Phenomena
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Multiplicity fluctuations in hadronic final states from the decay of the Z0

1992

An analysis of the fluctuations in the phase space distribution of hadrons produced in the decay of 78829 Z0 has been carried out, using the method of factorial moments. The high statistics collected by the DELPHI experiment at LEP during 1990 allowed studies of the event sample both globally and in intervals of p(t) and multiplicity, and for different jet topologies and for single jets. A large contribution to the factorial moments of the one-dimensional data on rapidity with respect to the event axis comes from hard gluons. Details of factorial moments in two and three dimensions are presented. Influences of resonance decays have been studied by Monte Carlo simulation: one-dimensional fac…

Nuclear and High Energy PhysicsFactorialParticle physicsE+E ANNIHILATIONLUND MONTE-CARLOMonte Carlo methodPartonMULTIPARTICLE PRODUCTION01 natural sciences7. Clean energyJET FRAGMENTATIONNuclear physicsParticle decayRAPIDITY DISTRIBUTIONS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RapidityZ0010306 general physicsParton showerHIGH-ENERGY COLLISIONSQuantum chromodynamicsPhysics010308 nuclear & particles physicsLUND MONTE-CARLO; HIGH-ENERGY COLLISIONS; E+E ANNIHILATION; MULTIPARTICLE PRODUCTION; RAPIDITY DISTRIBUTIONS; INTERMITTENCY ANALYSIS; JET FRAGMENTATION; Z0; QCD; SIMULATIONQCDINTERMITTENCY ANALYSISGluonSIMULATIONHigh Energy Physics::ExperimentFísica nuclearParticle Physics - Experiment
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The cosmic ray proton plus helium energy spectrum measured by the ARGO-YBJ experiment in the energy range 3-300 TeV

2015

The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray Observatory (Tibet, People's Republic of China, 4300 m a.s.l.). The high altitude, combined with the full-coverage technique, allows the detection of extensive air showers in a wide energy range and offer the possibility of measuring the cosmic ray proton plus helium spectrum down to the TeV region, where direct balloon/space-borne measurements are available. The detector has been in stable data taking in its full configuration from November 2007 to February 2013. In this paper the measurement of the cosmic ray proton plus helium energy spectrum is presented in the region 3-300 TeV by analyzi…

Nuclear and High Energy PhysicsPARTICLE-ACCELERATIONPhysics and Astronomy (miscellaneous)ProtonAstrophysics::High Energy Astrophysical PhenomenaSHELLFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesUltra-high-energy cosmic ray010306 general physicsCosmic-ray observatoryDETECTORNuclear and High Energy PhysicPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSSpectral index010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityAir shower13. Climate actionSUPERNOVA REMNANTHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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