Search results for "Wide band"

showing 10 items of 31 documents

Generation of white LED light by frequency downconversion using a perylene-based dye

2012

A high efficiency white light emitting diode (LED) was fabricated by generation of frequency down-conversion from a GaN/InGaN blue LED. In place of conventional inorganic phosphors, a perylene-based dye was used for colour conversion. The resulting hybrid structure is analysed by focusing on the visual performance of the realised LEDs employing the most relevant photometric parameters of a light source. Preparation of the organic polymer is described as well. The thermal stability of the dye was investigated and a simple structure which avoids colour degradation is proposed.

Organic polymerMaterials sciencebusiness.industryPhosphordyes light emitting diodes phosphors polymers wide band gap semiconductors GaN-InGaN blue LED colour conversionSettore ING-INF/01 - Elettronicalaw.inventionchemistry.chemical_compoundOpticsLight sourcechemistrylawOptoelectronicsDegradation (geology)Thermal stabilityElectrical and Electronic EngineeringbusinessPeryleneDiodeLight-emitting diode
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Correlation between Zn vacancies and photoluminescence emission in ZnO films.

2006

Photoluminescence and positron annihilation spectroscopy have been used to characterize and identify vacancy-type defects produced in ZnO films grown on sapphire by metal-organic chemical-vapor deposition. The photoluminescence of the samples in the near band edge region has been studied, paying particular attention to the emission at 370.5 nm (3.346 eV). This emission has been correlated to the concentration of Zn vacancies in the films, which has been determined by positron annihilation spectroscopy. Jesus.Zuniga@uv.es Vicente.Munoz@uv.es

PhotoluminescenceMaterials scienceAstrophysics::High Energy Astrophysical PhenomenaEdge regionAnalytical chemistrySemiconductor thin filmsGeneral Physics and AstronomyPositron annihilation spectroscopyCondensed Matter::Materials Science:FÍSICA [UNESCO]Zinc compoundsMetalorganic vapour phase epitaxyDeposition (law)Positron annihilationCondensed matter physicsCondensed Matter::OtherPhysicsWide-bandgap semiconductorpositron annihilationUNESCO::FÍSICACacancies (crystal)II-VI semiconductorsWide band gap semiconductorsZn vacanciesMOCVDSapphireZnOphotoluminescenceZinc compounds ; II-VI semiconductors ; Wide band gap semiconductors ; Semiconductor thin films ; Positron annihilation ; Cacancies (crystal) ; MOCVD
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Optical characterization of Mg-doped GaN films grown by metalorganic chemical vapor phase deposition

2000

Scanning electron microscopy, micro-Raman, and photoluminescence (PL) measurements are reported for Mg-doped GaN films grown on (0001) sapphire substrates by low-pressure metalorganic chemical vapor phase deposition. The surface morphology, structural, and optical properties of GaN samples with Mg concentrations ranging from 1019 to 1021 cm−3 have been studied. In the scanning micrographs large triangular pyramids are observed, probably due to stacking fault formation and three-dimensional growth. The density and size of these structures increase with the amount of magnesium incorporated in the samples. In the photoluminescence spectra, intense lines were found at 3.36 and 3.31 eV on the tr…

PhotoluminescenceMaterials scienceIII-V semiconductorsScanning electron microscopeAnalytical chemistryGeneral Physics and AstronomySemiconductor thin filmsChemical vapor depositionStacking faultsSurface topographysymbols.namesake:FÍSICA [UNESCO]MagnesiumGallium compounds ; III-V semiconductors ; Wide band gap semiconductors ; Magnesium ; Semiconductor thin films ; MOCVD coatings ; Scanning electron microscopy ; Raman spectra ; Photoluminescence ; Surface composition ; Surface topography ; Stacking faults ; Inclusions ; ExcitonsPhotoluminescenceWurtzite crystal structureDopingUNESCO::FÍSICAGallium compoundsWide band gap semiconductorsMOCVD coatingsSurface compositionInclusionssymbolsSapphireExcitonsRaman spectraRaman spectroscopyScanning electron microscopyStacking fault
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Modulation of the electronic properties of GaN films by surface acoustic waves

2003

We report on the interaction between photogenerated electron-hole pairs and surface acoustic waves (SAW) in GaN films grown on sapphire substrates. The spatial separation of photogenerated carriers by the piezoelectric field of the SAW is evidenced by the quenching of the photoluminescence (PL) intensity. The quenching levels in GaN are significantly smaller than those measured in GaAs under similar conditions. The latter is attributed to the lower exciton ionization efficiency and carrier separation probabilities mediated by the piezoelectric effect. The PL spectra also evidence energy shifts and broadenings of the electronic transitions, which are attributed to the band gap modulation by …

PhotoluminescenceMaterials scienceIII-V semiconductorsSurface acoustic wavesBand gapExcitonRadiation quenchingGeneral Physics and AstronomySemiconductor thin filmsCondensed Matter::Materials Science:FÍSICA [UNESCO]IonizationPiezoelectric semiconductorsPhotoluminescenceQuenchingbusiness.industryUNESCO::FÍSICAWide-bandgap semiconductorGallium compoundsAcoustic waveCondensed Matter::Mesoscopic Systems and Quantum Hall EffectWide band gap semiconductorsGallium compounds ; III-V semiconductors ; Wide band gap semiconductors ; Surface acoustic waves ; Semiconductor thin films ; Photoluminescence ; Radiation quenching ; Piezoelectric semiconductors ; Excitons ; Energy gapEnergy gapSapphireOptoelectronicsExcitonsbusiness
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The TESS Grand Unified Hot Jupiter Survey I. 10 planets

2022

Hot Jupiters-short-period giant planets-were the first extrasolar planets to be discovered, but many questions about their origin remain. NASA's Transiting Exoplanet Survey Satellite (TESS), an all-sky search for transiting planets, presents an opportunity to address these questions by constructing a uniform sample of hot Jupiters for demographic study through new detections and unifying the work of previous ground-based transit surveys. As the first results of an effort to build this large sample of planets, we report here the discovery of 10 new hot Jupiters (TOI-2193Ab, TOI-2207b, TOI-2236b, TOI-2421b, TOI-2567b, TOI-2570b, TOI-3331b, TOI-3540Ab, TOI-3693b, TOI-4137b). All of the planets…

Photometryobservational astronomyRadial velocityAstrophysics and AstronomyExoplanetsPhysicsexoplanet astronomyWide-band photometryNatural SciencesInfrared photometrySpectroscopyWide band photometryOptical astronomy
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Failure analysis of normally-off GaN HEMTs under avalanche conditions

2020

Gallium nitride (GaN) high electron-mobility transistors (HEMTs) are promising devices in the power electronics field owing to their wide bandgap (WBG). However, all the potential advantages provided by their WBG require reliability improvement. In industrial applications, robustness is one of the main factors considered by circuit designers. This study focuses on the observation of the degradation behavior of the main waveforms of unclamped inductive-switching (UIS) test circuits of two different commercial GaN HEMT structures. The relevance of this study lies in the potential applications of these devices to high-voltage applications and automotive systems where they are subjected to many…

Power HEMTMaterials scienceIII-V semiconductorswide band gap semiconductorsbusiness.industryoutagesion beamsNormally offCondensed Matter Physicshigh electron mobility transistorsAvalanche breakdownElectronic Optical and Magnetic MaterialsMaterials ChemistryOptoelectronicsimpact ionizationElectrical and Electronic Engineeringbusinessgallium nitride
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Rateless Codes Performance Analysis in Correlated Channel Model for GEO Free Space Optics Downlinks

2012

Settore ING-INF/03 - TelecomunicazioniFree Space Optics (FSO) technologies for satellite communications offer several advantages: wide bandwidth high rate capability immunity to electromagnetic interference and small equipment size. Thus they are suitable for inter-satellite links deep space communications and also for high data rate ground-to-satellite/satellite-to-ground communications. Nevertheless FSO links suffer impairments that cause power signal degradation at the receiver. Scattering and absorption cause power signal attenuations predictable by suitable deterministic models. Optical turbulence causes random irradiance fluctuations which can generate signal fading events and can thereby only be predicted by statistical models. Attenuation and fading events can corrupt FSO links and so it would be recommended to add mitigation error codes on the communication link. FSO channel can be described as an erasure channel: fading events can cause erasure errors. We have identified in rateless codes (RCs) a suitable solution to be employed in FSO links. RCs do not need feedback and they add a redundant coding on the source data that allows the receiver to recover the whole payload despite erasure errors. We implemented two different of rateless codes: Luby Transform (LT) and Raptor. We analyzed their performances on a simulated turbulent GEO FSO downlink (1 Gbps - OOK modulation) at a 106 μm wavelength and for different values of zenith angles. Assuming a plane-wave propagation and employing Hufnagel-Valley we modeled the downlink using: 1) a temporal correlated channel model based on Gamma-Gamma probability distribution and 2) an irradiance covariance function that we converted on a time function using Taylor frozen eddies hypothesis. Our new channel model is able to simulate irradiance fluctuations at different turbulence conditions as it will be shown in the full paper. We will also report performance results of LT and Raptor codes at overhead range varying between 0 and 50% and for different values of source packets.Settore ING-INF/01 - Elettronica
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Natural optical anisotropy of h-BN: Highest giant birefringence in a bulk crystal through the mid-infrared to ultraviolet range

2018

The giant birefringence of layered h-BN was demonstrated by analyzing the interference patterns in reflectance and transmittance measurements in the mid-infrared to the deep ultraviolet energy range. The refractive index for polarization perpendicular to the c axis is much higher than the refractive index for polarization parallel to the c axis, and it displays a strong increase in the ultraviolet range that is attributed to the huge excitonic effects arising from the unique electronic structure of h-BN. Thus, h-BN is shown to exhibit a giant negative birefringence that ranges from -0.7 in the visible to -2 in the deep ultraviolet close to the band gap. The electronic dielectric constants f…

Van der waals interactionsRefractive-IndexMaterials sciencePhysics and Astronomy (miscellaneous)Band gap02 engineering and technologyDielectricsemiconductorsmedicine.disease_cause01 natural sciencesMolecular physicswide bandgapHeterostructures constants0103 physical sciencesmedicineTransmittancePressureHexagonalGeneral Materials SciencePlane010306 general physicsAnisotropyBirefringenceGAASSystems021001 nanoscience & nanotechnologyPolarization (waves)2D materialsBoron nitride[PHYS.COND.CM-GEN]Physics [physics]/Condensed Matter [cond-mat]/Other [cond-mat.other][PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Single-crystalsGraphene0210 nano-technologyRefractive indexUltraviolet
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Photometry of candidate members of NGC6611

2009

We present the list of candidate members of the young open cluster NGC 6611, selected in a field of view of 33'x34' by the X-rays emission and excesses in infrared bands. X-ray sources without infrared excesses are classified as candidate Class III cluster members; stars with infrared excesses as disk bearing members. Cone search capability for table J/A+A/496/453/catalog (NGC 6611 cluster member positions and magnitudes)

observational astronomyOpen star clustersPhotometryAstrophysics and AstronomyStellar AstronomyPhysicsWide-band photometryNatural SciencesInfrared photometryWide band photometryOptical astronomy
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VRIJHK observations of PKS 2155-304

2008

Spectral variability is the main tool for constraining emission models of BL Lac objects. By means of systematic observations of the BL Lac prototype PKS 2155-304 in the infrared-optical band, we explore variability on the scales of months, days and hours. We made our observations with the robotic 60cm telescope REM located at La Silla, Chile. VRIJHK filters were used. PKS 2155-304 was observed from May to December 2005. The wavelength interval explored, the total number of photometric points and the short integration time render our photometry substantially superior to previous ones for this source. On the basis of the intensity and colour we distinguish three different states of the sourc…

observational astronomyPhotometrygalactic and extragalactic astronomyAstrophysics and AstronomyPhysicsBL Lacertae objectsWide-band photometryNatural SciencesInfrared photometryWide band photometryOptical astronomy
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