Search results for "Glas"

showing 10 items of 1259 documents

Solidification behavior of the theta system 2-propanol/poly(n-butyl methacrylate) I. Influences of thermoreversible gelation on stationary flow

1994

Zero shear viscosities, η0, were determined by means of a magnetoviscometer for melts of poly(n-butyl methacrylate) (M = 8.7 to 450 kg/mol, T =53.5 to 200°C) and for concentrated solutions of the highest molecular weight sample in isopropanol (T = 34.8 to 131.5 °C). Master curves can be constructed in both cases if the reference temperature is set proportional to the gelation temperature of the particular fluid. Special intersegmental interactions (eventually leading to thermoreversible gelation) can above all be felt in η0 (T) and in M c , the critical molecular weight determined in plots of log η0 vs. log M. As the temperature is lowered, the behavior changes from WLF to Arrhenius, and M …

Arrhenius equationMaterials scienceTheta solventThermodynamicsCondensed Matter PhysicsMethacrylatePoly n-butyl methacrylatePropanolShear (sheet metal)symbols.namesakechemistry.chemical_compoundchemistryPolymer chemistrysymbolsStationary flowGeneral Materials ScienceGlass transitionRheologica Acta
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Dipolar and orientational glass formation in two-dimensional films of CO mixtures

2002

Heat-capacity and dielectric measurements have been performed to study orientational and dipolar order and disorder phenomena in submonolayer films of CO and binary mixtures of CO physisorbed on graphite and boron nitride (BN). With both methods transitions to quadrupolar and dipolar ordered low-temperature phases have been found for pure CO. Calorimetric measurements revealed that the dipolar transition of CO on graphite belongs to the universality class of the two-dimensional (2D) Ising model. It will be shown that in dilute mixtures of CO with CH 4 molecules a dramatic suppression of this phase transition occurs. This effect turned out to be much stronger than that previously observed in…

Arrhenius equationPhase transitionCondensed matter physicsChemistryDielectricCondensed Matter PhysicsElectronic Optical and Magnetic Materialssymbols.namesakechemistry.chemical_compoundBoron nitrideImpurityChemical physicsMaterials ChemistryCeramics and CompositessymbolsIsing modelGraphiteOrientational glassJournal of Non-Crystalline Solids
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Fragmentation of polycarbonate macroinitiators in solution and in the bulk state

1990

The diphenylethane initiator 3,4-diethyl-3,4-(p-methoxyphenyl)-hexane (T–OCH3) was synthesized. By cocondensation of bisphenol A or C and the bisphenol derivative (“T”) of T–OCH3 with phosgene, polycarbonate macroinitiators PC(TxA1-x) and PC(TxC1-x) with different compositions x were made. The thermal fragmentation of T–OCH3 and the copolycarbonates was investigated with and without a radical scavenger both in solution and in the bulk state. The primary dissociation of T–OCH3 is a monomolecular Arrhenius process with a characteristic temperature of T* (τ = 1h) = 140°C (τ: average life time of the intact molecule). When the radicals are not intercepted, the dissociation is excessively revert…

Arrhenius equationPolymers and PlasticsChemistryRadicalActivation energyCondensed Matter PhysicsDissociation (chemistry)symbols.namesakeFragmentation (mass spectrometry)visual_artPolymer chemistryMaterials Chemistryvisual_art.visual_art_mediumsymbolsPhysical and Theoretical ChemistryPolycarbonateRadical disproportionationGlass transitionJournal of Polymer Science Part B: Polymer Physics
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Diverging Collectives: Artist-Run Spaces versus Warehouse Shows Comparative models of art production and cooperation among young British artists

2017

The paper addresses the case of artist-run spaces and warehouse shows in the United Kingdom between the 1980s and 1990s, a time when autonomous group shows and independent artist collectives sprawled particularly thanks to the engagement of a new generation of artists, among whom were found later celebrities such as Damien Hirst and Douglas Gordon. It will be argued that both artist-run spaces and warehouse shows were feasible solutions for young authors against art market barriers and economic crisis, although they held structural and organisational differences that would affect aesthetic outcomes and present art history with a shift in the model of the art collective.

Artist-Run Spaces Warehouse Shows Douglas Gordon Damien Hirst young British artistsDouglas GordonDamien Hirstyoung British artistsSettore M-FIL/04 - EsteticaArtist-Run SpacesSettore L-ART/03 - Storia dell'Arte ContemporaneaWarehouse ShowsArtist-Run Spaces Warehouse Shows Douglas Gordon Damien Hirst
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Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

2017

On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently by the Fermi Gamma-ray Burst Monitor, and the Anticoincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory. The probability of the near-simultaneous temporal and spatial observation of GRB 170817A and GW170817 occurring by chance is $5.0\times 10^{-8}$. We therefore confirm binary neutron star mergers as a progenitor of short GRBs. The association of GW170817 and GRB 170817A provides new insight into fundamental physics and the origin of short gamma-ray bursts. We use the ob…

AstrofísicaGravitacióneutron star: binaryclose [binaries]Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]BATSE OBSERVATIONSgamma-ray burst: generalEQUIVALENCE PRINCIPLEEXTENDED EMISSIONastro-ph.HE; astro-ph.HEAstrophysicsKilonovageneral [gamma-ray burst]01 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologyphoton: velocityPROMPT EMISSIONLIGOclose gamma-ray burst: general gravitational waves [binaries]gravitational wave010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)BURST SPECTRAQCQBPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)binaries: closeGRBEQUATION-OF-STATEviolation: Lorentzgamma ray: emissiongravitational wavesAstrophysics - High Energy Astrophysical PhenomenaGWradiation: electromagneticAfterglow Light CurvesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstinvariance: LorentzGW GRB LIGO Virgo Fermi BNSGLASTOptical Afterglows0103 physical sciencesgamma ray: detectorBinaries: close; gamma-ray burst: general; gravitational wavesSTFCFermi010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKAstronomy and AstrophysicsAstronomy and Astrophysictime delaysensitivityShapiro delayLIGORedshiftNeutron starVIRGOPhysics and AstronomyHOST GALAXYCPT VIOLATION13. Climate actiongravitationSpace and Planetary ScienceLUMINOSITY FUNCTIONVIEWING ANGLEbinaries: close; gamma-ray burst: general; gravitational waves; Astronomy and Astrophysics; Space and Planetary ScienceBNSspectrometerGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]redshift: measuredFermi Gamma-ray Space TelescopeAstrophysical Journal Letters
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Multifrequency Studies of the Peculiar Quasar 4C +21.35 during the 2010 Flaring Activity

2014

著者人数: 290名

AstrofísicaelectronPhotontorusAstrophysics01 natural scienceslaw.inventiongalaxies: active – gamma rays: general – quasars: general – quasars: individual (4C +21.35) – radiation mechanisms: non-thermalactive gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermal [galaxies]lawblack hole: Kerrgalaxies: active; gamma rays: general; quasars: general; quasars: individual: 4C +21.35; radiation mechanisms: non-thermalopticalGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsenergy: highPhysicsphotonRadiusnon-thermal [radiation mechanisms]Synchrotrongamma ray: emissionactive [galaxies]astro-ph.COElectrónicaFísica nuclearElectricidadGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal; Nuclear and High Energy PhysicsAstrophysics - High Energy Astrophysical Phenomenaquasars: individual (4C +21.35)Astrophysics - Cosmology and Nongalactic AstrophysicsFlareradiation mechanisms: non-thermal; galaxies: active; quasars: general; quasars: individual (4C +21.35); gamma rays: observationsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAAstrophysics::High Energy Astrophysical Phenomenaeducationgalaxies: activeFOS: Physical sciencesquasars: individual: 4C +21.35Astrophysics::Cosmology and Extragalactic AstrophysicsVHEGLASTemission: modelTelescopeX-rayquasars: general0103 physical sciencessynchrotrongalaxies: active gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermalquasarflux: densityindividual: 4C +21.35 [quasars]Astrophysics::Galaxy AstrophysicsAstronomia Observacionsgeneral [quasars]010308 nuclear & particles physicsAstronomy and AstrophysicsQuasargamma rays: generalradiation mechanisms: non-thermalAstrophysics - Astrophysics of GalaxiesMAGICRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)ddc:520spectral[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [gamma rays]Fermi Gamma-ray Space Telescope
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An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray …

2018

A new analysis of the dataset from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ultra-high-energy cosmic rays on an intermediate angular scale, which is indicative of excess arrivals from strong, nearby sources. The data consist of 5514 events above 20 EeV with zenith angles up to 80 deg recorded before 2017 April 30. Sky models have been created for two distinct populations of extragalactic gamma-ray emitters: active galactic nuclei from the second catalog of hard Fermi-LAT sources (2FHL) and starburst galaxies from a sample that was examined with Fermi-LAT. Flux-limited samples, which include all types of galaxies from the Swift-BAT and 2MASS …

Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ciencias Físicascosmic radiation: densitygalaxies: starburstAstrophysics01 natural sciences//purl.org/becyt/ford/1 [https]methods: data analysis Supporting material: FITS fileUltra-high-energy cosmic raydata analysis [Methods]Anisotropycosmic radiation: model010303 astronomy & astrophysicscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files; Astronomy and Astrophysics; Space and Planetary ScienceAugerobservatorygamma ray: emissiondata analysis Supporting material: FITS file [methods]astroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical Phenomenagalaxies: activeData analysisFOS: Physical sciencesStarburstCosmic rayanisotropyAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias FísicasGLASTcosmic raysastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files0103 physical sciencesHigh Energy Physicscosmic radiation: UHEAGNCosmic raysAstrophysics::Galaxy AstrophysicsZenithmethods: data analysis Supporting material: FITS filesPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsIsotropyFísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Astronomy and Astrophysicmethods: data analysisGalaxyfluxstarburst [Galaxies]Space and Planetary ScienceExperimental High Energy PhysicsActive galaxiesgalaxyAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statistical
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Multiple accelerated particle populations in the Cygnus Loop with Fermi-LAT

2021

The Cygnus Loop (G74.0-8.5) is a very well-known nearby supernova remnant (SNR) in our Galaxy. Thanks to its large size, brightness, and angular offset from the Galactic plane, it has been studied in detail from radio to $\gamma$-ray emission. The $\gamma$ -rays probe the populations of energetic particles and their acceleration mechanisms at low shock speeds. We present an analysis of the $\gamma$-ray emission detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope over 11 years in the region of the Cygnus Loop. We performed detailed morphological and spectral studies of the $\gamma$-ray emission toward the remnant from 100 MeV to 100 GeV and compared it with X-ra…

Astrophysics::High Energy Astrophysical Phenomenabrightnesscosmic radiation: energyFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeV01 natural sciencesGLASTthermalX-raycosmic raysSpitzer Space Telescope0103 physical sciencesultravioletsupernovaRadiative transferopticalcloudcosmic radiation: acceleration010306 general physicsSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsacceleration of particlesISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cygnus LoopAstronomy and Astrophysicsshock wavesGalactic planeGalaxy13. Climate actionSpace and Planetary Sciencegamma raystatisticsspectralgalaxyAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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Bias correction of dynamically downscaled precipitation to compute soil water deficit for explaining year-to-year variation of tree growth over north…

2017

This paper documents the accuracy of a post-correction method applied to precipitation regionalized by the Weather Research and Forecasting (WRF) Regional Climate Model (RCM) for improving simulated rainfall and feeding impact studies. The WRF simulation covers Burgundy (northeastern France) at a 8-km resolution and over a 20-year long period (1989–2008). Previous results show a strong deficiency of the WRF model for simulating precipitation, especially when convective processes are involved. In order to reduce such biases, a Quantile Mapping (QM) method is applied to WRF-simulated precipitation using the mesoscale atmospheric analyses system SAFRAN («Système d'Analyse Fournissant des Rense…

Atmospheric Science010504 meteorology & atmospheric sciences0208 environmental biotechnologyméthode de correction02 engineering and technologybourgogneCOMMON BEECH01 natural sciencesCiencias de la Tierra y relacionadas con el Medio AmbienteWater balanceREGIONAL CLIMATE MODELLINGGlobal and Planetary Changedéficit hydriqueForestry[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyClimatologyWATER BALANCECommon beechSOIL WATER DEFICITFrance[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyCIENCIAS NATURALES Y EXACTASforêt tempéréeWRFMesoscale meteorology[ SDV.SA.SDS ] Life Sciences [q-bio]/Agricultural sciences/Soil study[SDV.SA.SDS]Life Sciences [q-bio]/Agricultural sciences/Soil studySpatial distributionDOUGLAS-FIRmedicineREGIONAL CLIMATE-CHANGE; ERA-INTERIM REANALYSIS; POTENTIAL IMPACT; TEMPERATE FOREST; FAGUS-SYLVATICA; SEVERE DROUGHT; MODEL; RESPONSES; SYSTEM; PROJECTIONSPrecipitationmodèle climatique[SDU.STU.HY]Sciences of the Universe [physics]/Earth Sciences/Hydrologyclimatologie régionaleWater balanceSoil water deficit0105 earth and related environmental sciencesQuantile mappingclimatprécipitationDouglas-firQUANTILE MAPPINGnord est de la France15. Life on landSeasonalitymedicine.disease020801 environmental engineering13. Climate actionWeather Research and Forecasting ModelSoil waterEnvironmental scienceClimate modelMeteorología y Ciencias Atmosféricas[ SDU.STU.HY ] Sciences of the Universe [physics]/Earth Sciences/HydrologyAgronomy and Crop ScienceRegional climate modelling
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MZ-35, a new layered pentasil borosilicate synthesized in the presence of large alkali cations

2013

Abstract A new layered borosilicate has been synthesized in the presence of cesium and sodium cations and its structure has been solved by a combination of automated diffraction tomography (ADT) and X-ray powder diffraction (XRPD). MZ-35 has a composition NaCs 2 [BSi 7 O 16 (OH) 2 ](OH) 2 ·4H 2 O and features space group P-4m2. The unusually small unit cell ( a 7.3081 A, c 10.7520 A) is shared by two random-stacked configurations of the structure: a network of connected pentasil units related to the layer of RUB-18 and a bidimensional checkerboard of intersecting ladders of 4-membered rings. The two configurations are related by the simple face-sharing inversion of a hydroxyl-bearing tetrah…

Automated electron diffraction tomography; Rietveld structure refinement; Layered borosilicate; 4-MR ladders; Face-sharing terahedraMaterials science4-MR laddersSodiumchemistry.chemical_element02 engineering and technology010402 general chemistry01 natural sciencesDiffraction tomographyFace-sharing terahedraGroup (periodic table)General Materials ScienceRietveld structure refinementLayered borosilicateBorosilicate glassAutomated electron diffraction tomographyGeneral Chemistry4-MR ladders; Automated electron diffraction tomography; Face-sharing terahedra; Layered borosilicate; Rietveld structure refinement[CHIM.MATE]Chemical Sciences/Material chemistry021001 nanoscience & nanotechnologyCondensed Matter PhysicsAlkali metal4-MR ladders; Automated electron diffraction tomography; Face-sharing terahedra; Layered borosilicate; Rietveld structure refinement;0104 chemical sciencesCrystallographychemistryMechanics of MaterialsCaesiumTetrahedron0210 nano-technologyPowder diffraction
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