Search results for "SPECTRA"

showing 10 items of 3542 documents

Spectral index-flux relation for investigating the origins of steep decay in γ-ray bursts

2020

$\gamma$-ray bursts (GRBs) are short-lived transients releasing a large amount of energy ($10^{51}-10^{53} $ erg) in the keV-MeV energy range. GRBs are thought to originate from internal dissipation of the energy carried by ultra-relativistic jets launched by the remnant of a massive star's death or a compact binary coalescence. While thousands of GRBs have been observed over the last thirty years, we still have an incomplete understanding of where and how the radiation is generated in the jet. Here we show a relation between the spectral index and the flux found by investigating the X-ray tails of bright GRB pulses via time-resolved spectral analysis. This relation is incompatible with the…

Photon010504 meteorology & atmospheric sciencesScienceAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFluxAstrophysicsRadiation7. Clean energy01 natural sciencesArticleGeneral Biochemistry Genetics and Molecular BiologyTransient astrophysical phenomena0103 physical sciencesAdiabatic process010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsJet (fluid)Spectral indexRange (particle radiation)MultidisciplinaryQGeneral Chemistrygamma-ray bursts steep decayHigh-energy astrophysicsAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstNature Communications
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Reflection component in the Bright Atoll Source GX 9+9

2020

GX 9+9 (4U 1728-16) is a low mass X-ray binary (LMXB) source harboring a neutron star. Although it belongs to the subclass of the bright Atoll sources together with GX 9+1, GX 3+1, and GX 13+1, its broadband spectrum is poorly studied and apparently does not show reflection features in the spectrum. To constrain the continuum well and verify whether a relativistic smeared reflection component is present, we analyze the broadband spectrum of GX 9+9 using {\it BeppoSAX} and \textit{XMM-Newton} spectra covering the 0.3-40 keV energy band. We fit the spectrum adopting a model composed of a disk-blackbody plus a Comptonized component whose seed photons have a blackbody spectrum (Eastern Model). …

PhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsColor temperature010502 geochemistry & geophysics01 natural sciencesSpectral lineX-rays: binariesstars: neutronAccretion accretion diskSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesBlack-body radiation010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)accretion disksAstronomy and AstrophysicsX-rays: binarieAccretion (astrophysics)Neutron starSpace and Planetary ScienceElectron temperatureAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLow Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]stars: individual: GX 9+9
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QUADRUPOLAR CHARACTER OF THE Ti K-EDGE PREPEAKS IN TiO2 BY RESONANT AUGER

2002

Resonant spectroscopies offer a new opportunity to get more insight into excited electronic states by studying line shapes and intensities of decay processes. For photon excitations in the pre-K-edge region, the Ti KL 2,3 L 2,3 Auger spectra in TiO 2 show additional peaks when an electron is promoted in localized d-like states via a quadrupolar transition. This resonant process is used to unravel the respective contributions of quadrupolar and dipolar transitions to the absorption edge prepeaks.

PhotonChemistrySurfaces and InterfacesElectronCondensed Matter PhysicsSpectral lineSurfaces Coatings and FilmsAugerDipoleK-edgeAbsorption edgeMaterials ChemistryAtomic physicsLine (formation)Surface Review and Letters
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Tailoring the transmittance of integrated optical waveguides with short metallic nanoparticle chains

2004

We study the ability of noble metal nanoparticle chains supporting localized surface plasmons to tailor the transmittance of channel waveguides on which they are deposited. The optical interaction between a microwaveguide ~MWG! and various arrangements of nanoparticles is first analyzed by means numerical calculations based on the Green’s tensor formalism. For specific geometries of the particle chains, the transmission spectra of the composite device ~MWG and nanoparticles! exhibits strong modulations in the optical range with the appearance of a neat band gap. The results of an experiment inspired by this theoretical study are also discussed. The photon scanning tunneling microscope image…

PhotonMaterials scienceBand gapbusiness.industryPhysics::OpticsNanoparticleCondensed Matter PhysicsSpectral lineElectronic Optical and Magnetic Materialslaw.inventionOpticslawTransmittanceQuasiparticleOptoelectronicsScanning tunneling microscopebusinessLocalized surface plasmonPhysical Review B
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Quantification of spatial inhomogeneity in perovskite solar cells by hyperspectral luminescence imaging

2016

Vacuum evaporated perovskite solar cells with a power conversion efficiency of 15% have been characterized using hyperspectral luminescence imaging. Hyperspectral luminescence imaging is a novel technique that offers spectrally resolved photoluminescence and electroluminescence maps (spatial resolution is 2 micrometer) on an absolute scale. This allows, using the generalized Planck’s law, the construction of absolute maps of the depth-averaged quasi-Fermi level splitting (Δμ), which determines the maximum achievable open circuit voltage (Voc) of the solar cells. In a similar way, using the generalized reciprocity relations the charge transfer efficiency of the cells can be obtained from the…

PhotonMaterials sciencePhotoluminescenceRenewable Energy Sustainability and the Environmentbusiness.industryOpen-circuit voltageEnergy conversion efficiencyHyperspectral imaging02 engineering and technology010402 general chemistry021001 nanoscience & nanotechnology01 natural sciencesPollution0104 chemical sciencesOpticsNuclear Energy and EngineeringEnvironmental ChemistryOptoelectronics0210 nano-technologyLuminescencebusinessAbsolute scalePerovskite (structure)Energy & Environmental Science
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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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