Search results for "HIGH-ENERGY"

showing 10 items of 161 documents

Reactivity of H2S and H2S/H2 Mixture With Molybdenum Oxide Thin Films Epitaxied on CoO (100) : Characterization by Rheed and Auger Spectroscopy

2010

Molybdenum-Cobalt composite oxide films were prepared by the evaporation of molybdenum trioxide on a fresh cleaved CoO (100) surface (Thickness = 10 A). The MoO3-CoO interface has been characterized simultaneously by reflexion high electron diffraction (RHEED) and Auger Electron Spectroscopy (AES). The thin film structure and composition depend on the annealing temperature. After a 300°C treatment, metallic cobalt islands nucleate at the interface thin film - CoO (100) and crystallize with the cubic FCC symmetry. After a 700°C treatment cobalt molybdate (a CoMoO4) islands grow. The metastable crystallites are epitaxied on CoO (100). After a 900°C treatment, the thin film consists of flat tw…

Auger electron spectroscopyCrystallographychemistry.chemical_compoundReflection high-energy electron diffractionChemistrychemistry.chemical_elementGeneral ChemistryCrystalliteThin filmMolybdateCobaltAmorphous solidMolybdenum trioxideBulletin des Sociétés Chimiques Belges
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Effect of the surface stoichiometry on the interaction of Mo with TiO2 (110)

2000

Abstract Molydenum has been deposited at room temperature on (110) TiO2 surfaces with different stoichiometries, roughnesses and crystallinities. Whatever the substrate preparation is, in-situ Auger electron spectroscopy (AES) and X-ray photoelectron spectroscopy (XPS) studies as well as ex-situ atomic force microscopy (AFM) and reflexion high-energy electron diffraction (RHEED) studies reveal a Stranski–Krastanov growth mode: the completion of three monolayers followed by islands growth is observed in every case. The three monolayers are always composed of amorphous molybdenum oxide with an oxidation state of molybdenum less than IV. The oxidation of the molybdenum layers generates Ti3+ an…

Auger electron spectroscopyReflection high-energy electron diffractionChemistryAnalytical chemistrychemistry.chemical_elementSurfaces and InterfacesSubstrate (electronics)Condensed Matter PhysicsElectron beam physical vapor depositionSurfaces Coatings and FilmsCrystallographyX-ray photoelectron spectroscopyElectron diffractionMolybdenumMonolayerMaterials ChemistrySurface Science
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Search for neutral heavy leptons produced in Z decays

1997

Weak isosinglet Neutral Heavy Leptons ($\nu_m$) have been searched for using data collected by the DELPHI detector corresponding to $3.3\times 10^{6}$ hadronic~Z$^{0}$ decays at LEP1. Four separate searches have been performed, for short-lived $\nu_m$ production giving monojet or acollinear jet topologies, and for long-lived $\nu_m$ giving detectable secondary vertices or calorimeter clusters. No indication of the existence of these particles has been found, leading to an upper limit for the branching ratio $BR($Z$^0\rightarrow \nu_m \overline{\nu})$ of about $1.3\times10^{-6}$ at 95\% confidence level for $\nu_m$ masses between 3.5 and 50 GeV/$c^2$. Outside this range the limit weakens rap…

COLLISIONSParticle physicsE+E ANNIHILATIONPhysics and Astronomy (miscellaneous)Electron–positron annihilationHadronMASSJet (particle physics)HIGH-ENERGY-PHYSICS; MONOJET PRODUCTION; E+E ANNIHILATION; MONTE-CARLO; BOSON; LIMITS; MASS; LEP; PERFORMANCE; COLLISIONSHIGH-ENERGY-PHYSICS01 natural sciences7. Clean energyMONOJET PRODUCTIONNuclear physicsLIMITSMONTE-CARLO0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsDELPHIBosonPhysics010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyBOSONLEPPERFORMANCELARGE ELECTRON POSITRON COLLIDERPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderPARTICLE PHYSICSHigh Energy Physics::ExperimentNeutrinoParticle Physics - ExperimentLepton
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The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

2018

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the…

Cherenkov Telescope ArrayHigh-energy astrophysical phenomenaCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomyenergy resolution7. Clean energy01 natural sciencesSpace missionlaw.inventionIceCubeEinstein TelescopelawObservatoryLIGO010303 astronomy & astrophysicsKM3NeTPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Applied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionGamma-ray astronomyGamma-ray polarizationCondensed Matter Physicsphoton: energyobservatoryNuclear astrophysicsApace missionAstrophysics - High Energy Astrophysical Phenomenaperformancedetector: technologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstspace missionCompton and pair creation telescopeTelescope0103 physical sciencessupernovaElectroniccalorimetergamma ray: detectorOptical and Magnetic MaterialsKAGRAElectrical and Electronic Engineering010306 general physicsTime domain astronomyLISAGamma-ray astronomyEinstein TelescopeAstronomyInstitut für Physik und AstronomieTime-domain astronomyCherenkov Telescope ArraysensitivityLIGOmessengerKM3NeTVIRGO13. Climate actionCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineeringddc:520galaxyCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic Engineering[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Correlation between Regional Atp and Blood Flow in Tumors and Surrounding Normal Tissue

1994

Various experimental and human tumors are characterized by a marked heterogeneity in the pathophysiologic micromilieu (1, 2). An inadequate and heterogeneous nutritional blood supply has been suggested to explain the non-uniform distribution of oxygen, pH, and high energy phosphates as it has been observed by many investigators (3, 4). Although there is a distinct understanding of the general interrelationships between these parameters (5), little is known about their actual regional correlation, which cannot be assessed by global measurements. With the autoradiographic method for measurement of blood flow (6, 7) and the metabolic imaging with ATP-induced bioluminescence (8, 9) it has becom…

CorrelationHigh-energy phosphatePathologymedicine.medical_specialtyMelanomamedicineNormal tissueDistribution (pharmacology)HamsterBlood flowBiologymedicine.diseasePathophysiology
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Size-dependent alignment of Fe nanoparticles upon deposition onto W(110)

2010

Using in situ electron diffraction we study the orientation of mass-selected iron nanoparticles upon deposition onto single crystalline W(110) at room temperature. It is found that particles with a diameter below about 4 nm and a kinetic energy $\ensuremath{\le}0.1$ electron volt per atom spontaneously align with respect to the substrate. Larger particles preferentially rest with their (001) and (110) facets parallel to the surface, but do not show further alignment. The data may hint at thermally activated dislocation motions upon the impact on the substrate which are responsible for the observed orientation below 4 nm. By this uniformly oriented monodisperse nanostructures can be prepared…

CrystallographyNanostructureReflection high-energy electron diffractionMaterials scienceElectron diffractionAtomNanoparticleSubstrate (electronics)DislocationCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsElectron backscatter diffractionPhysical Review B
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Timing techniques applied to distributed modular high-energy astronomy: the H.E.R.M.E.S. project

2021

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy concept. Conceived as a mini-constellation of six 3U nano-satellites hosting a new miniaturized detector, HERMES-TP/SP aims at the detection and accurate localisation of bright high-energy transients such as Gamma-Ray Bursts. The large energy band, the excellent temporal resolution and the wide field of view that characterize the detectors of the constellation represent the key features for the next generation high-energy all-sky monitor with good localisation capabilities that will play a pivotal role in the future …

CubeSatsHigh energyHigh-energy astronomyReal-time computingFOS: Physical sciences01 natural sciences7. Clean energy010309 opticsX-rays0103 physical sciencesNano-satellitesTemporal triangulationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsConstellationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsModular designPathfinderTemporal resolutionGamma Ray BurstsTransient (oscillation)Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
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BART: The Czech Autonomous Observatory

2010

The High Energy Astrophysics group of the stellar department of the Astronomical Institute in Ondřejov operates two small aperture robotic telescopes called BART and D50. Both telescopes are capable of making automatic followup observation of gamma-ray burst optical counterparts. This paper deals with the smaller telescope BART.

CzechPhysicsHigh-energy astronomylcsh:AstronomyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrophysicsLarge apertureAstrophysics::Cosmology and Extragalactic Astrophysicslanguage.human_languagelaw.inventionTelescopelcsh:QB1-991Space and Planetary ScienceObservatorylawlanguageAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsAdvances in Astronomy
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Using Electron Diffraction to Solve the Crystal Structure of a Laked Azo Pigment

2009

The structure of the ζ phase of Pigment Red 53:2 was solved using electron diffraction data. The unit cell determination appeared to be more complicated due to twinning of the crystals. A series of...

DiffractionCrystallographyReflection high-energy electron diffractionElectron diffractionGas electron diffractionChemistryGeneral Materials ScienceGeneral ChemistryCrystal structureCondensed Matter PhysicsCrystal twinningCrystallographic defectElectron backscatter diffractionCrystal Growth & Design
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Electron diffraction, X-ray powder diffraction and pair-distribution-function analyses to determine the crystal structures of Pigment Yellow 213, C23…

2009

The crystal structure of the nanocrystalline alpha phase of Pigment Yellow 213 (P.Y. 213) was solved by a combination of single-crystal electron diffraction and X-ray powder diffraction, despite the poor crystallinity of the material. The molecules form an efficient dense packing, which explains the observed insolubility and weather fastness of the pigment. The pair-distribution function (PDF) of the alpha phase is consistent with the determined crystal structure. The beta phase of P.Y. 213 shows even lower crystal quality, so extracting any structural information directly from the diffraction data is not possible. PDF analysis indicates the beta phase to have a columnar structure with a si…

DiffractionModels MolecularAza CompoundsReflection high-energy electron diffractionChemistryMolecular ConformationGeneral MedicineCrystal structurePair-distribution functionHeterocyclic Compounds 4 or More RingsGeneral Biochemistry Genetics and Molecular BiologyPigment Yellow 213CrystalCrystallinityCrystallographyElectron diffractionElectron diffractionMicroscopy Electron TransmissionX-ray powder diffractionElectron diffraction; Pair-distribution function; Pigment Yellow 213; X-ray powder diffractionParticle SizeColoring AgentsPowder diffractionPowder DiffractionElectron backscatter diffractionActa crystallographica. Section B, Structural science
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