Search results for "Spectral"

showing 10 items of 3116 documents

Modeling spectral correlations of photon-pairs generated in liquid-filled photonic crystal fiber

2020

The generation of photon-pairs with controllable spectral correlations is crucial in quantum photonics. Here we present the design of a photonic crystal fiber to generate widely-spaced four-wave mixing bands with spectral correlations that can be tuned through the thermo-optic effect after being infiltrated with heavy water. We present a theoretical study of the purity of the signal (idler) photon generated as a function of temperature, pump spectral linewidth and the length of the fiber. 511-6/18-8876 CIIC155/2019 APN-624 TEC2016- 76664-C2-1-R PROMETEO/2019/048

PhotonMaterials sciencephoton sourcesbusiness.industryUNESCO::FÍSICANonlinear opticsPhysics::OpticsSignalAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialsnon-linear opticsspectral correlationsLaser linewidthOptics:FÍSICA [UNESCO]OptoelectronicsFibermicrostructured optical fibersPhotonicsbusinessQuantumPhotonic-crystal fiber
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Gamma Ray Spectrum from Thermal Neutron Capture on Gadolinium-157

2018

International audience; We have measured the |$\gamma$|-ray energy spectrum from the thermal neutron capture, |${}^{157}$|Gd|$(n,\gamma)$|⁠, on an enriched |$^{157}$|Gd target (Gd|$_{2}$|O|$_{3}$|⁠) in the energy range from 0.11 MeV up to about 8 MeV. The target was placed inside the germanium spectrometer of the ANNRI detector at J-PARC and exposed to a neutron beam from the Japan Spallation Neutron Source (JSNS). Radioactive sources (⁠|$^{60}$|Co, |$^{137}$|Cs, and |$^{152}$|Eu) and the |$^{35}$|Cl(⁠|$n$|⁠,|$\gamma$|⁠) reaction were used to determine the spectrometer‘s detection efficiency for |$\gamma$| rays at energies from 0.3 to 8.5 MeV. Using a Geant4-based Monte Carlo simulation of …

PhotonPhysics - Instrumentation and DetectorsMonte Carlo methodGeneral Physics and Astronomy7. Clean energy01 natural sciencesnuclear reactionSpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)H43 Software architectures[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]n: fissionNuclear Experiment (nucl-ex)n: captureNuclear ExperimentNuclear ExperimentPhysicsdensityJ-PARC LabphotonGamma rayInstrumentation and Detectors (physics.ins-det)Atomic physicsnumerical calculations: Monte CarloSpallation Neutron SourceNeutron captureAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumchemistry.chemical_elementFOS: Physical sciencesGermanium[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]n: thermalF20 Instrumentation and technique0103 physical sciencesModels of nuclear reactions[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutron capture gamma ray cascade Models of nuclear reactions Neutrinos from supernova remnant010306 general physicsD21 Models of nuclear reactionsgamma ray cascadeSpectrometer010308 nuclear & particles physicsnucleusNeutron radiationH20 Instrumentation for underground experiments* Automatic Keywords *germaniumF22 Neutrinos from supernova remnant and other astronomical objectschemistryn: beamNeutrinos from supernova remnantefficiencygamma rayspectrometerC43 Underground experimentsgadolinium
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Spectral evolution of superluminal components in parsec-scale jets

2008

27 pages, 18 figures, 1 table, 1 appendix.-- Pre-print archive.

PhotonRadiation mechanisms: non-thermalAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysicsRelativitysymbols.namesakeAstrophysical jetRadiative transfereducationPhysicseducation.field_of_studySpectral indexnon-thermal [Radiation mechanisms]Superluminal motionAstrophysics (astro-ph)Astronomy and AstrophysicsMagnetic fieldLorentz factorGalaxies: jetsSpace and Planetary ScienceHydrodynamicssymbolsjets [Galaxies]
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Subpicosecond transient signal spectroscopy of Prodan in dimethylformamide solution.

2008

We report a pump-probe experiment revealing the temporal evolution of subpicosecond evolution of Prodan's excited-state absorption in dimethylformamide. Also, we present calculation of the first spectral moment of this spectral band and estimation of different relaxation components on the subpicosecond time scale.

PhotonsModels StatisticalTime FactorsChemistryPhotochemistryGeneral NeuroscienceLasersRelaxation (NMR)Analytical chemistryDimethylformamideSpectral bandsEquipment DesignMolecular physicsGeneral Biochemistry Genetics and Molecular BiologyAbsorptionchemistry.chemical_compoundKineticsSpectrometry FluorescenceHistory and Philosophy of Science2-NaphthylamineDimethylformamideSpectroscopyAbsorption (electromagnetic radiation)Transient signalFluorescent DyesAnnals of the New York Academy of Sciences
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Hyperspectral terahertz microscopy via nonlinear ghost imaging

2020

Ghost imaging, based on single-pixel detection and multiple pattern illumination, is a crucial investigative tool in difficult-to-access wavelength regions. In the terahertz domain, where high-resolution imagers are mostly unavailable, ghost imaging is an optimal approach to embed the temporal dimension, creating a “hyperspectral” imager. In this framework, high resolution is mostly out of reach. Hence, it is particularly critical to developing practical approaches for microscopy. Here we experimentally demonstrate time-resolved nonlinear ghost imaging, a technique based on near-field, optical-to-terahertz nonlinear conversion and detection of illumination patterns. We show how space–time c…

Physics - Instrumentation and DetectorsComputer scienceTerahertz radiationFOS: Physical sciences02 engineering and technologyGhost imaging01 natural sciences010309 opticssymbols.namesakeOptics0103 physical sciencesMicroscopyCouplingbusiness.industryQC0454.T47Hyperspectral imagingInstrumentation and Detectors (physics.ins-det)QC0446.2021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsQC0350Electronic Optical and Magnetic MaterialsNonlinear systemWavelengthFourier transformComputer Science::Computer Vision and Pattern Recognitionsymbols0210 nano-technologybusinessOptics (physics.optics)Physics - Optics
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Gamma Ray Spectra from Thermal Neutron Capture on Gadolinium-155 and Natural Gadolinium

2019

Natural gadolinium is widely used for its excellent thermal neutron capture cross section, because of its two major isotopes: $^{\rm 155}$Gd and $^{\rm 157}$Gd. We measured the $\gamma$-ray spectra produced from the thermal neutron capture on targets comprising a natural gadolinium film and enriched $^{\rm 155}$Gd (in Gd$_{2}$O$_{3}$ powder) in the energy range from 0.11 MeV to 8.0 MeV, using the ANNRI germanium spectrometer at MLF, J-PARC. The freshly analysed data of the $^{\rm 155}$Gd(n, $\gamma$) reaction are used to improve our previously developed model (ANNRI-Gd model) for the $^{\rm 157}$Gd(n, $\gamma$) reaction, and its performance confirmed with the independent data from the $^{\r…

Physics - Instrumentation and DetectorsGadoliniumMonte Carlo methodAnalytical chemistryenergy spectrumGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesGermanium[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]n: thermal7. Clean energy01 natural sciencesSpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)F20 Instrumentation and technique0103 physical sciencesH43 Software architectures[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)n: capture010306 general physicsNuclear ExperimentMonte CarloPhysicsD21 Models of nuclear reactionsIsotopeSpectrometer010308 nuclear & particles physicsJ-PARC LabGamma rayInstrumentation and Detectors (physics.ins-det)Gadolinium neutron capture gamma ray cascadeNeutron temperature3. Good healthparticle: interactionH20 Instrumentation for underground experimentsgermaniumF22 Neutrinos from supernova remnant and other astronomical objectsC42 Reactor experimentschemistrygamma rayC43 Underground experimentsspectrometergadoliniumperformance
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Continuous-wave cavity ring-down polarimetry

2020

We present a new cavity-based polarimetric scheme for highly sensitive and time-resolved measurements of birefringence and dichroism, linear and circular, that employs rapidly pulsed single-frequency continuous wave (CW) laser sources and extends current cavity-based spectropolarimetric techniques. We demonstrate how the use of a CW laser source allows for gains in spectral resolution, signal intensity, and data acquisition rate compared to traditional pulsed-based cavity ring-down polarimetry (CRDP). We discuss a particular CW-CRDP modality that is different from intensity-based cavity-enhanced polarimetric schemes as it relies on the determination of the polarization rotation frequency du…

Physics - Instrumentation and DetectorsPolarimetryGeneral Physics and AstronomyFOS: Physical sciencesApplied Physics (physics.app-ph)010402 general chemistry01 natural scienceslaw.inventionFinessesymbols.namesakeOpticslawPhysics - Chemical Physics0103 physical sciencesFaraday effectddc:530Physical and Theoretical ChemistrySpectral resolutionPhysicsChemical Physics (physics.chem-ph)Birefringence010304 chemical physicsbusiness.industryPhysics - Applied PhysicsInstrumentation and Detectors (physics.ins-det)LaserPolarization (waves)0104 chemical sciencesPhysics - Atmospheric and Oceanic PhysicsAtmospheric and Oceanic Physics (physics.ao-ph)symbolsContinuous wavebusinessPhysics - OpticsOptics (physics.optics)
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Comparison of proton shower developments in the BGO calorimeter of the Dark Matter Particle Explorer between GEANT4 and FLUKA simulations

2020

The DArk Matter Particle Explorer (DAMPE) is a satellite-borne detector for high-energy cosmic rays and $\gamma$-rays. To fully understand the detector performance and obtain reliable physical results, extensive simulations of the detector are necessary. The simulations are particularly important for the data analysis of cosmic ray nuclei, which relies closely on the hadronic and nuclear interactions of particles in the detector material. Widely adopted simulation softwares include the GEANT4 and FLUKA, both of which have been implemented for the DAMPE simulation tool. Here we describe the simulation tool of DAMPE and compare the results of proton shower properties in the calorimeter from t…

Physics - Instrumentation and DetectorsProton85Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHadronDark matterS-General Physics and AstronomyFOS: Physical sciencesCosmic rayNuclear physicsSpectral analysisInstrumentation and Methods for Astrophysics (astro-ph.IM)Monte Carlo simulationPhysicsTp9550Calorimeter (particle physics)96DetectorInstrumentation and Detectors (physics.ins-det)5513Cosmic Rays-n-tParticleHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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Evolution of correlation structure of industrial indices of U.S. equity markets

2013

We investigate the dynamics of correlations present between pairs of industry indices of US stocks traded in US markets by studying correlation based networks and spectral properties of the correlation matrix. The study is performed by using 49 industry index time series computed by K. French and E. Fama during the time period from July 1969 to December 2011 that is spanning more than 40 years. We show that the correlation between industry indices presents both a fast and a slow dynamics. The slow dynamics has a time scale longer than five years showing that a different degree of diversification of the investment is possible in different periods of time. On top to this slow dynamics, we als…

Physics - Physics and SocietyIndex (economics)Scale (ratio)Operations researchSettore SECS-P/05Diversification (finance)FOS: Physical sciencesPhysics and Society (physics.soc-ph)01 natural sciences010305 fluids & plasmasFOS: Economics and businessCorrelationRandom matrix theoryMINIMUM SPANNING-TREES0103 physical sciencesEconometricsPCA Random matrix theory010306 general physicsCORRELATION-BASED NETWORKSMathematicsPCAStatistical Finance (q-fin.ST)Settore SECS-S/03CROSS-CORRELATIONSCovariance matrixSpectral propertiesSettore SECS-S/06Equity (finance)Quantitative Finance - Statistical FinanceFINANCIAL-MARKETSSubprime crisisInvestment (macroeconomics)Degree (music)Settore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)DYNAMIC ASSET TREESMATRICES
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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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