Search results for "620"

showing 10 items of 203 documents

Dual Luminescence, Interligand Decay, and Nonradiative Electronic Relaxation of Cyclometalated Iridium Complexes in Solution

2016

Femtosecond broadband photoluminescence studies are presented for Ir(ppy)3 (Ir1), Ir(ppy)2(pic) (Ir2), Ir(ppy)2(bpy)(PF6) (Ir3), Ir(ppz)3 (Ir4), and Ir(ppz)2dipy (Ir5) (where ppy = 2-phenylpyridine, pic = picolinate, bpy = 2,2′-bipyridine, ppz = 1-phenylpyrazole, and dipy = 5-phenyldipyrrinato) in solution. Upon 400-nm excitation of Ir1–Ir3, we observed a prompt population of the lowest MLCT states. The higher states decay on an ultrafast time scale (3MLCT state undergoes further vibrational relaxation on a 1-ps time scale. In Ir3, this relaxation is accompanied by an interligand decay from the ppy to the bpy ligand in ∼1.5 ps. For the ppy-containing complexes (Ir1 and Ir2), we found that, …

Photoluminescence530 PhysicsPopulationSurfaces Coatings and Filmchemistry.chemical_element02 engineering and technology010402 general chemistryPhotochemistry01 natural sciences540 ChemistryVibrational energy relaxationIridiumPhysical and Theoretical Chemistryeducationeducation.field_of_studyElectronic Optical and Magnetic MaterialRelaxation (NMR)620 Engineering021001 nanoscience & nanotechnology0104 chemical sciencesSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsEnergy (all)General EnergychemistryFemtosecond0210 nano-technologyLuminescenceExcitationThe Journal of Physical Chemistry C
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Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina -Comision Nacional de Energia Atomica; Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT); Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargue; NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia -the Australian Research Council; Braz…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstronomyPerformance of High Energy Physics Detector01 natural sciences7. Clean energyEtc)030218 nuclear medicine & medical imaging0302 clinical medicineFront-end electronics for detector readoutAPDsInstrumentationphysics.ins-detPhoton detectors for UVMathematical PhysicsInstrumentation et méthodes en physiqueEBCCDsVisible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)electronicsSettore FIS/01 - Fisica SperimentaleCalibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UVPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsInstrumentation and Detectors (physics.ins-det)charged particleAPDs; Calibration and fitting methods; Performance of High Energy Physics Detectors; Photon detectors for UV; CCDs; Cluster finding; CMOS imagers; EBCCDs; EMCCDs; Etc); Front-end electronics for detector readout; Pattern recognition; G-APDs; Si-PMTs; Visible and IR photons (solid-state) (PIN diodesAugerobservatorydensity [muon]Pattern recognition cluster finding calibration and fitting methodG-APDsChristian ministryupgradeddc:620Astrophysics - Instrumentation and Methods for Astrophysicsperformanceatmosphere [showers]Land accessCherenkov counter: waterairAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesPolitical sciencePattern recognition0103 physical sciencesmuon: densityFront-end electronics for detector readout; Pattern recognitionphotomultiplier: siliconHigh Energy Physicscosmic radiation: UHE[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610CMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Engineering & allied operationsscintillation counterCalibration and fitting methodsshowers: atmosphere010308 nuclear & particles physicswater [Cherenkov counter]Cluster findingAutres mathématiquesCCDsEMCCDsResearch councilefficiencyExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::ExperimentHumanitiesRAIOS CÓSMICOSastro-ph.IM
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The energy spectrum of cosmic rays beyond the turn-down around 1017 eV as measured with the surface detector of the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina – Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia – the Australian Research Council; Be…

Physics and Astronomy (miscellaneous)AstronomyAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesFluxCosmic rayAstrophysics7. Clean energy01 natural sciencesdetector: fluorescenceAugercosmic rayssurface [detector]Observatory0103 physical sciencescalorimeterddc:530High Energy Physicscosmic radiation: UHEspectrum [cosmic radiation]010303 astronomy & astrophysicsEngineering (miscellaneous)Engineering & allied operationsHigh Energy Astrophysical Phenomena (astro-ph.HE)fluorescence [detector]Pierre Auger ObservatoryPhysicsastro-ph.HEcosmic radiation: energy spectrumcosmic radiation: spectrumdetector: surface010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugerCalorimeterfluxobservatoryspectralddc:620[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenaenergy spectrum [cosmic radiation]Energy (signal processing)RAIOS CÓSMICOSultra-high energy cosmic rays energy spectrum features.
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Elastic waves propagation in 1D fractional non-local continuum

2008

Aim of this paper is the study of waves propagation in a fractional, non-local 1D elastic continuum. The non-local effects are modeled introducing long-range central body interactions applied to the centroids of the infinitesimal volume elements of the continuum. These non-local interactions are proportional to a proper attenuation function and to the relative displacements between non-adjacent elements. It is shown that, assuming a power-law attenuation function, the governing equation of the elastic waves in the unbounded domain, is ruled by a Marchaud-type fractional differential equation. Wave propagation in bounded domain instead involves only the integral part of the Marchaud fraction…

PhysicsNon-local elasticityContinuum mechanicsWave propagationDifferential equationMathematical analysisCondensed Matter PhysicsFractional calculuDispersion of elastic waves; Lattice models; Long-range interactions; Non-local elasticity; Fractional calculus; Fractional power lawPower lawAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsFractional calculusLattice modelLove waveLong-range interactionIngenieurwissenschaftenDispersion of elastic waveBounded functionddc:620Settore ICAR/08 - Scienza Delle CostruzioniLongitudinal waveFractional power law
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The MuPix high voltage monolithic active pixel sensor for the Mu3e experiment

2015

Mu3e is a novel experiment searching for charged lepton flavor violation in the rare decay μ → eee. In order to reduce background by up to 16 orders of magnitude, decay vertex position, decay time and particle momenta have to be measured precisely. A pixel tracker based on 50 μm thin high voltage monolithic active pixel sensors (HV-MAPS) in a magnetic field will deliver precise vertex and momentum information. Test beam results like an excellent efficiency of >99.5% and a time resolution of better than 16.6 ns obtained with the MuPix HV-MAPS chip developed for the Mu3e pixel tracker are presented.

PhysicsParticle physicsCMOS sensorElectronic detector readout concepts (solid-state)PixelPhysics::Instrumentation and Detectorsbusiness.industryHigh voltageChipElectronic detector readout concepts (solid-state); Particle tracking detectors (solidstate detectors)Magnetic fieldVertex (geometry)OpticsHigh Energy Physics::Experimentddc:610Electric potentialDetectors and Experimental TechniquesParticle tracking detectors (solidstate detectors)ddc:620businessInstrumentationParticle Physics - ExperimentMathematical PhysicsEngineering & allied operationsLepton
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Space-, time- and spin-resolved photoemission

2015

Journal of electron spectroscopy and related phenomena 200, 94 - 118 (2015). doi:10.1016/j.elspec.2015.05.016

PhysicsRadiationbusiness.industrySpace timeDegrees of freedom (physics and chemistry)Spin engineeringPosition and momentum spaceAngle-resolved photoemission spectroscopyElectronCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsComputational physics620MomentumOpticsPhysical and Theoretical Chemistryddc:620businessSpectroscopySpin-½
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On the numerical scheme employed in gyrotron interaction simulations

2012

We report on the influence of the numerical scheme employed in gyrotron interaction simulations. Results obtained with the Crank-Nicolson scheme are compared with those obtained with the Backward Time – Centred Space (BTCS) fully implicit scheme. We present realistic cases where, for discretisation parameters in the range usually used in gyrotron simulations, the results can be very different. Hence, the numerical scheme used can be responsible for obscuring the underlying physics if its convergence is not tested carefully.

PhysicsScheme (programming language)DiscretizationPhysicsQC1-999Space (mathematics)law.inventionlawGyrotronConvergence (routing)Range (statistics)Statistical physicsddc:620computerEngineering & allied operationscomputer.programming_language
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A dynamic collimation and alignment system for the Helmholtz linear accelerator

2021

Review of scientific instruments 92(11), 113306 - 113306-9 (2021). doi:10.1063/5.0069824

Physicsbusiness.industryCollimated lightLinear particle accelerator620Transverse planesymbols.namesakeOpticsCryomoduleHelmholtz free energysymbolsContinuous wavePhysics::Accelerator PhysicsThermal emittanceddc:620businessInstrumentationBeam (structure)
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Field and numerical study of river confluence flow structures

2010

River hydrodynamics Turbulent open channel flow and transport phenomena

Physics::Fluid DynamicsPhysics::Space PhysicsIngenieurwissenschaften (620)Numerical simulation Large Eddy simulation HydrodynamicsPhysics::Atmospheric and Oceanic PhysicsComputer Science::Information TheoryPhysics::Geophysics
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

2020

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers.

Physics::Instrumentation and DetectorsAstronomyprimary [cosmic radiation]01 natural sciences030218 nuclear medicine & medical imagingAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinesurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Data Processing; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of High Energy Physics DetectorsInstrumentationMathematical PhysicsData Processing; Large detector systems for particle and astroparticle physics; Largedetector-systems performance; Performance of High Energy Physics DetectorsLarge detector-systems performanceHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEInstrumentation et méthodes en physiqueData ProcessingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugercascadeobservatoryCascadeLargedetector-systems performanceddc:620Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airAstrophysics::High Energy Astrophysical PhenomenawaterFOS: Physical sciencesCosmic rayAtmosphere03 medical and health sciencesOptics0103 physical sciencesHigh Energy Physics14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithEngineering & allied operationsPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryhep-exdetector: surfaceLarge detector systems for particle and astroparticle physicsAutres mathématiquescosmic radiation: primaryCherenkov counterExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentPerformance of High Energy Physics Detectorsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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