Search results for "COALESCENCE"

showing 10 items of 92 documents

The influence of AlN buffer over the polarity and the nucleation of self-organized GaN nanowires

2015

We experimentally investigate the influence of AlN buffer growth on the nucleation and the polarity of a self-organized assembly of GaN nanowires (NWs) grown on Si. Two complementary growth mechanisms for AlN buffer deposited on Si are demonstrated. Both emphasize the aggregation of Si on the AlN surface and the growth of large cubic crystallites, namely, AlN pedestals. Further growths of GaN NWs assembly reveal that the GaN 2D layer found at the bottom of the NW assembly is the result of the coalescence of Ga-polar pyramids, whereas AlN pedestals are observed as preferential but not exclusive NW nucleation sites. NWs are N-polar or exhibit inversion domains with a Ga-polar core/N-polar she…

010302 applied physicsCoalescence (physics)[PHYS]Physics [physics]Materials sciencebusiness.industryNucleationWide-bandgap semiconductorNanowireGeneral Physics and AstronomyNanotechnology02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesBuffer (optical fiber)Nanolithography0103 physical sciencesOptoelectronicsCrystalliteSelf-assembly0210 nano-technologybusinessComputingMilieux_MISCELLANEOUS
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Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart

2020

We study the impact of gas accretion on the orbital evolution of black-hole binaries initially at large separation in the band of the planned Laser Interferometer Space Antenna (LISA). We focus on two sources: (i)~stellar-origin black-hole binaries~(SOBHBs) that can migrate from the LISA band to the band of ground-based gravitational-wave observatories within weeks/months; and (ii) intermediate-mass black-hole binaries~(IMBHBs) in the LISA band only. Because of the large number of observable gravitational-wave cycles, the phase evolution of these systems needs to be modeled to great accuracy to avoid biasing the estimation of the source parameters. Accretion affects the gravitational-wave p…

010504 meteorology & atmospheric sciencesAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)Observableastro-ph.HE; astro-ph.HE; General Relativity and Quantum Cosmologygas: accretionblack holes gravitational wavesobservatoryInterferometrygravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenainterferometermedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational radiation: direct detectionelectromagnetic field: productionGeneral Relativity and Quantum Cosmologybinary: coalescencestatistical analysisSettore FIS/05 - Astronomia e Astrofisicagravitation: weak field0103 physical sciencesnumerical calculationsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLISAGravitational wavegravitational radiationOrder (ring theory)black hole: accretionAstronomy and Astrophysicsblack holesgravitational radiation detectorRedshiftBlack holeblack hole: binarySpace and Planetary ScienceSkygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray: detectorThe Astrophysical Journal
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Micro magnetofluidics: droplet manipulation of double emulsions based on paramagnetic ionic liquids

2013

The ability to control and manipulate discrete fluid droplets by magnetic fields offers new opportunities in microfluidics. A surfactant-free and easy to realize technique for the continuous generation of double emulsion droplets, composed of an organic solvent and a paramagnetic ionic liquid, is applied. The inner phase of the emulsion droplet consists of imidazolium-based ionic liquids with either iron, manganese, nickel or dysprosium containing anions which provide paramagnetic behaviour. The double emulsion droplets are dispersed in a continuous phase of FC-40. All substances - the organic phase, the paramagnetic ionic liquid and the continuous phase -are immiscible. The magnetic proper…

AnionsIronMicrofluidicsMicrofluidicsBiomedical EngineeringMixing (process engineering)Analytical chemistryIonic LiquidsBioengineeringBiochemistryPhysics::Fluid DynamicsMagneticsParamagnetismchemistry.chemical_compoundNickelPhase (matter)DysprosiumPhysics::Atomic and Molecular ClustersCoalescence (physics)ManganeseChemistryImidazolesGeneral ChemistryMagnetic fieldCondensed Matter::Soft Condensed MatterChemical engineeringMagnetIonic liquidEmulsionshuman activitiesLab on a Chip
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GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

2019

We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1$\mathrm{M}_\odot$ during the first and second observing runs of the Advanced gravitational-wave detector network. During the first observing run (O1), from September $12^\mathrm{th}$, 2015 to January $19^\mathrm{th}$, 2016, gravitational waves from three binary black hole mergers were detected. The second observing run (O2), which ran from November $30^\mathrm{th}$, 2016 to August $25^\mathrm{th}$, 2017, saw the first detection of gravitational waves from a binary neutron star inspiral, in addition to the observation of gravitational waves from a total of seven binary …

AstrofísicaDYNAMICSGravitacióneutron star: binaryAstronomyGeneral Physics and AstronomyBinary numberAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010305 fluids & plasmasgravitational waves black holesAstrophysicSIGNALSPopulation DistributionsLIGOQCQBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HESettore FIS/01gravitational radiation detector: networkPROGENITORSPhysicsgravitational wavesPhysical Sciencesastro-ph.CO[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaMETALLICITYAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)QC1-999gr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsMASSAstrophysics; GravitationGeneral Relativity and Quantum CosmologyBinary black holebinary: coalescenceSYSTEMS0103 physical sciences010306 general physicsSTFCScience & TechnologyGravitational wavegravitational radiationRCUKGravitational Wave Physicsbinary: compactLIGOEVOLUTIONBlack holeNeutron starVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionBLACK-HOLERADIATIONINFERENCE[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Search for eccentric binary black hole mergers with advanced LIGO and advanced Virgo during their first and second observing runs

2019

When formed through dynamical interactions, stellar-mass binary black holes may retain eccentric orbits ($e>0.1$ at 10 Hz) detectable by ground-based gravitational-wave detectors. Eccentricity can therefore be used to differentiate dynamically-formed binaries from isolated binary black hole mergers. Current template-based gravitational-wave searches do not use waveform models associated to eccentric orbits, rendering the search less efficient to eccentric binary systems. Here we present results of a search for binary black hole mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo. The search uses min…

AstrofísicaGravitació010504 meteorology & atmospheric sciencesIMPACTAstronomyWAVESBinary numberAstrophysicsgravitational waves; black hole; LIGO; VirgoLIGO-Virgo01 natural sciencesRendering (computer graphics)GravitationElliptical orbitCOMPACT-OBJECT BINARIESblack holeEccentricCOMPACT-OBJECT BINARIES; YOUNG STAR-CLUSTERS; EVOLUTION; PERTURBATIONS; PROGENITORS; IMPACT;WAVESEccentricity (behavior)LIGO010303 astronomy & astrophysicsorbitQCmedia_commonQBSettore FIS/01PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PROGENITORSAstrophysical black holesGravitational waves; Elliptical orbits; Astrophysical black holesPERTURBATIONSJustice and Strong Institutionsgravitational wavesPhysical SciencesAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaYOUNG STAR-CLUSTERSGravitational wavedata analysis methodSDG 16 - Peacemedia_common.quotation_subjectGravitational waves Elliptical orbits Astrophysical black holesFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsGravitational wavesElliptical orbitsGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black holebinary: coalescencestatistical analysis0103 physical sciencesWaveformSTFC0105 earth and related environmental sciencesScience & Technologybinary: formationVirgoSDG 16 - Peace Justice and Strong Institutionsgravitational radiationRCUKAstronomy and Astrophysics/dk/atira/pure/sustainabledevelopmentgoals/peace_justice_and_strong_institutionsLIGOEVOLUTIONgravitational radiation detectordetector: sensitivityVIRGOPhysics and Astronomyblack hole: binarySpace and Planetary Sciencegravitational radiation: emissioneccentric BBHstar: mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

2019

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gravitational-wave transients with a duration of milliseconds to approximately one second in the 32-4096 Hz frequency band with minimal assumptions about the signal properties, thus targeting a wide variety of sources. We also perform a matched-filter search for gravitational-wave transients from cosmic string cusps for which the waveform is well-modeled. The unmodeled search detected gravitational waves from several binary black hole mergers which have been identified by previous analyses. No other significant event…

AstronomyGravitational waves detectionAstrophysicsdetector: network01 natural sciencesSignalGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational waves detection Stochastic gravitational-wavebinary [black hole]LIGOgravitational waveQCQBmedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsgravitational waves neutron starsgravitational wavesGeneral relativityburst [gravitational radiation]network [detector]Physical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]direct detection [gravitational radiation]Advanced VirgoAstrophysics - High Energy Astrophysical PhenomenaFrequency bandsensitivity [detector]gr-qcmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalternative theories of gravityGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionemission [gravitational radiation]Binary black holeSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesgravitational radiation: burstAdvanced LIGOWaveformddc:530010306 general physicscosmic stringSTFCScience & Technology010308 nuclear & particles physicsGravitational waveRCUKStochastic gravitational-waveGravitational Wave PhysicsLIGOgravitational radiation detectorgravitational waves; Advanced LIGO; Advanced VirgoCosmic stringdetector: sensitivityVIRGOPhysics and Astronomyblack hole: binarySkygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikcoalescence [binary][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The dynamics of slug trains in volcanic conduits: Evidence for expansion driven slug coalescence

2017

Strombolian volcanism is a ubiquitous form of activity, driven by the ascent and bursting of bubbles of slug morphology. Whilst considerable attention has been devoted to understanding the behaviour of individual slugs in this regime, relatively little is known about how inter-slug interactions modify flow conditions. Recently, we reported on high temporal frequency strombolian activity on Etna, in which the larger erupted slug masses were followed by longer intervals before the following explosion than the smaller bursts (Pering et al., 2015). We hypothesised that this behaviour arose from the coalescence of ascending slugs causing a prolonged lag before arrival of the next distinct bubble…

Basaltic degassingBasaltic degassing; Slug coalescence; Slug dynamics; Strombolian volcanism; Geophysics; Geochemistry and PetrologyGeochemistry and PetrologySlug dynamicStrombolian volcanismSlug coalescenceGeophysicSettore GEO/08 - Geochimica E Vulcanologia
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Post-fragmentation vesiculation timescales in hydrous rhyolitic bombs from Chaitén volcano

2020

Abstract Bubble nucleation and growth dynamics exert a primary control on the explosivity of volcanic eruptions. Numerous theoretical and experimental studies aim to capture the complex process of melt vesiculation, whereas textural studies use vesicle populations to reconstruct magma behaviour. However, post-fragmentation vesiculation in rhyolitic bombs can create final quenched bubble (vesicle) textures that are not representative of the nature of fragmenting magma within the conduit. To examine bubble growth in hydrous rhyolitic bombs, we have used heated stage microscopy to directly observe vesiculation of a Chaiten rhyolite melt (with an initial dissolved water content of ~0.95 wt %) a…

Coalescence (physics)010506 paleontologyVulcanian eruptionBubbleClose-packing of equal spheresGeologyVolcanic explosivity index010502 geochemistry & geophysics01 natural sciencesRhyoliteGrowth ratePetrologyVolcanic bombGeology0105 earth and related environmental sciencesEarth-Surface ProcessesJournal of South American Earth Sciences
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Riming of Graupel: Wind Tunnel Investigations of Collection Kernels and Growth Regimes

2009

Abstract Laboratory experiments were carried out in the vertical wind tunnel in Mainz, Germany, to study the collision coalescence growth of single spherical ice particles having initial radii between 290 and 380 μm while they were freely floated in a laminar flow containing a cloud of supercooled droplets with radii between 10 and 20 μm. The experiments were performed in a temperature range between −8 and −12°C, where riming proceeds in the atmosphere, and with cloud liquid water contents lying between 0.9 and 1.6 g m−3 (i.e., values typically found in mixed-phase clouds). The collection kernels were calculated from the mass increase of the rimed ice particles and the average liquid water …

Coalescence (physics)Atmospheric ScienceMaterials scienceMeteorologyLiquid water contentLaminar flowAstrophysics::Earth and Planetary AstrophysicsMechanicsSupercoolingTemperature measurementGraupelWind tunnelIcingJournal of the Atmospheric Sciences
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Shapes and oscillations of raindrops with reduced surface tensions: Measurements at the Mainz vertical wind tunnel

2013

Abstract Important characteristics of raindrops pertinent to fields in atmospheric sciences such as weather radar or pollution scavenging are drop shape, oscillation frequency and amplitude, as well as the internal circulation. Atmospheric raindrops are never pure water drops but contain additional components like aerosol particles and dissolved species. Surface active substances, when present, reduce the surface tension of raindrops and, thus, increase the drop deformation which in turn affects breakup and coalescence, pollutant scavenging, and, finally, the formation of precipitation. Experiments were performed at the Mainz vertical wind tunnel with raindrops freely suspended at their ter…

Coalescence (physics)Atmospheric ScienceMaterials scienceTerminal velocitybusiness.industryOscillationDrop (liquid)MechanicsBreakupAerosolSurface tensionOpticsbusinessWind tunnelAtmospheric Research
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