Search results for "Degree of polarization"

showing 10 items of 22 documents

Reversed polarized emission in highly strained a-plane GaN/AlN multiple quantum wells

2010

The polarization of the emission from a set of highly strained $a$-plane GaN/AlN multiple quantum wells of varying well widths has been studied. A single photoluminescence peak is observed that shifts to higher energies as the quantum well thickness decreases due to quantum confinement. The emitted light is linearly polarized. For the thinnest samples the preferential polarization direction is perpendicular to the wurtzite $c$ axis with a degree of polarization that decreases with increasing well width. However, for the thickest well the preferred polarization direction is parallel to the $c$ axis. Raman scattering, x-ray diffraction, and transmission electron microscopy studies have been p…

010302 applied physicsPhysicsElectron densityCondensed matter physicsLinear polarizationOscillator strengthQuantum point contact: Physics [G04] [Physical chemical mathematical & earth Sciences]Infinitesimal strain theory02 engineering and technology021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesElectronic Optical and Magnetic MaterialsCondensed Matter::Materials Science: Physique [G04] [Physique chimie mathématiques & sciences de la terre]Quantum dotQuantum mechanics0103 physical sciences[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Degree of polarization0210 nano-technologyQuantum wellComputingMilieux_MISCELLANEOUS
researchProduct

Photophysical behavior of 3-methylquinoline and 3-bromoquinoline

1992

Abstract The phosphorescence emission and excitation spectra and their polarizations have been studied for 3-methylquinoline and 3-bromoquinoline in methylcyclohexane and ethanol glasses at 77 K. From the results obtained in 3-methylquinoline (τp = 1.30 s in ethanol, τp = 1.05 s in methylcyclohexane and the out-of-plane polarization) it is concluded that the emission originates from a triplet state of 3ππ∗ character. In 3-bromoquinoline, the phosphorescence lifetimes (ca. 8 ms in a non-polar solvent and 15 ms in a polar solvent) and the negative degree of polarization indicate an emitting state of ππ∗ character that is strongly coupled to a higher-lying triplet state of the nπ∗ type. The mo…

Absorption spectroscopyChemistryBiophysicsGeneral ChemistryCondensed Matter PhysicsPhotochemistryBiochemistryAtomic and Molecular Physics and OpticsSolventchemistry.chemical_compoundMoleculeDegree of polarizationMethylcyclohexaneTriplet statePolarization (electrochemistry)PhosphorescenceJournal of Luminescence
researchProduct

Anisotropic polarization of non‐polar GaN quantum dot emission

2009

We report on experimental and theoretical studies of the polarization selection rules of the emission of non-polar GaN/AlN self-assembled quantum dots. Time-integrated and time-resolved photoluminescence measurements have been performed to determine the degree of polarization. It is found that the emission of some samples can be predominantly polarized parallel to the wurtzite c axis, in striking difference with the previously reported results for bulk GaN and its heterostructures, in which the emission was preferentially polarized perpendicular to the c axis. Theoretical calculations based on an 8-band k·p model are used to analyze the relative importance of strain, confinement and quantum…

Condensed Matter::Materials SciencePhotoluminescenceCondensed matter physicsChemistryQuantum dotPerpendicularDegree of polarizationHeterojunctionCondensed Matter PhysicsAnisotropyPolarization (waves)Wurtzite crystal structurephysica status solidi c
researchProduct

Signatures of photon and axion-like particle mixing in the gamma-ray burst jet

2011

Photons couple to Axion-Like Particles (ALPs) or more generally to any pseudo Nambu-Goldstone boson in the presence of an external electromagnetic field. Mixing between photons and ALPs in the strong magnetic field of a Gamma-Ray Burst (GRB) jet during the prompt emission phase can leave observable imprints on the gamma-ray polarization and spectrum. Mixing in the intergalactic medium is not expected to modify these signatures for ALP mass > 10^(-14) eV and/or for < nG magnetic field. We show that the depletion of photons due to conversion to ALPs changes the linear degree of polarization from the values predicted by the synchrotron model of gamma ray emission. We also show that when …

High Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic fieldPhysicsPhotonAstrophysics::High Energy Astrophysical PhenomenaGamma rayFísicaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPolarization (waves)Synchrotronlaw.inventionMagnetic fieldPhysics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)lawDegree of polarizationGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena
researchProduct

Three-dimensional polarimetric computational integral imaging

2012

In this paper, we propose a novel 3D polarimetric computational integral imaging system by using polarization diversity of objects under natural illumination conditions. In the system, the measured Stokes polarization parameters are utilized to generate degree of polarization images of a 3D scene. Based on degree of polarization images and original 2D images, we utilize a modified computational reconstruction method to perform 3D polarimetric image reconstruction. The system may be used to detect or classify objects with distinct polarization signatures in 3D space. Experimental results also show the proposed system may mitigate the effect of occlusion in 3D reconstruction.

Integral imagingComputer sciencebusiness.industry3D reconstructionPolarimetryIterative reconstructionPolarization (waves)Atomic and Molecular Physics and OpticsOpticsComputer Science::Computer Vision and Pattern RecognitionDegree of polarizationImage sensorbusinessCircular polarizationOptics Express
researchProduct

Variability and polarization in the inner jet of 3C 395

2001

We present new results on the parsec-scale jet of the quasar 3C395, derived from VLBI polarization sensitive observations made in 1995.91 and 1998.50 at 8.4, 15.4 and 22.2 GHz. The observations show a complex one-sided jet extending up to 20 mas, with a projected magnetic field essentially aligned with the radio jet. The emission is strongly dominated, in total intensity and polarization, by the core and the inner jet region (of ~3 mas length). We have studied the details of this dominant region finding clear structural variations during this ~2.5 years period, in contrast with the apparent quietness of the jet structure inferred from lower resolution VLBI observations. We observe the eject…

InterferometricAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAsymbols.namesakeFaraday effectVery-long-baseline interferometryJetsPhysicsIndividual galaxiesAstrophysics (astro-ph)Active Galaxies ; Individual galaxies ; 3C 395 ; Jets ; Radio continuum ; InterferometricAstronomy and AstrophysicsQuasarPolarization (waves):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Magnetic fieldRadio continuumPolarization sensitiveSpace and Planetary Science3C 395symbolsDegree of polarizationUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaActive Galaxies:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

Scattering and Depolarization in a Polymer Dispersed Liquid Crystal Cell

2008

An imaging polarimeter in transmission has been used to explore the effects of scatter and depolarization induced by a polymer dispersed liquid crystal cell. The experiment was carried out for three visible wavelengths. Both a directional and a scattered component can be distinguished in the light transmitted by this material. Whereas the directional component increased with voltage, the scattered portion decreased. This was a common behaviour for all three wavelengths. The polarimetric analysis revealed that the degree of polarization was also affected by changes in the voltage applied to the cell. Depolarization effects in the scattered component were usually high and decreased with volta…

Materials sciencebusiness.industryScatteringPolarimeterDepolarizationCondensed Matter PhysicsElectronic Optical and Magnetic Materialssymbols.namesakeWavelengthOpticssymbolsStokes parametersDegree of polarizationbusinessVoltageVisible spectrumFerroelectrics
researchProduct

Polarization backward-wave four-wave mixing in BaTiO_3:Fe using the photovoltaic effect

1997

We report the first study to our knowledge of polarization backward-wave four-wave mixing in a BaTiO3:Fe crystal and compare the results of our measurements with the calculations performed within the model of photovoltaic charge transport. Two identically polarized pump waves and one orthogonally polarized signal wave are sent to a sample in a plane normal to the crystal’s C axis; a phase-conjugate wave with polarization identical to that of the signal wave is generated. With a 2-mm-thick sample a phase-conjugate reflectivity Rpc≈0.01 is reached; for a 1-cm-thick sample, amplified reflection should be possible.

Materials sciencebusiness.industryStatistical and Nonlinear PhysicsTransverse wavePhotovoltaic effectElliptical polarizationPolarization (waves)Atomic and Molecular Physics and OpticsFour-wave mixingOpticsCross-polarized wave generationDegree of polarizationAtomic physicsbusinessCircular polarizationJournal of the Optical Society of America B
researchProduct

Anisotropic photoluminescence of nonpolar ZnO epilayers and ZnO/Zn1 −xMgxO multiple quantum wells grown on LiGaO2 substrate

2020

Ministry of Science and Technology, Taiwan (104-2221-E-110-012-MY3, 107-2221-E-110-004-MY3); National Natural Science Foundation of China (51602309, U1605245).

PhotoluminescenceMaterials scienceCondensed matter physicsbusiness.industry02 engineering and technology021001 nanoscience & nanotechnologyPolarization (waves)01 natural sciences7. Clean energyAtomic and Molecular Physics and Optics010309 opticsCondensed Matter::Materials ScienceOptics0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]Degree of polarization0210 nano-technologybusinessLuminescenceAnisotropyElectronic band structureQuantum wellStacking fault
researchProduct

Messungen der Himmelsstrahlung und deren Polarisationsgrad während der Sonnenfinsternis am 15.2.1961 in Viareggio (Italien)

1961

On the occasion of the total solar eclipse in Viareggio (Italy) measurements of intensity of sky radiation and polarization have been carried out at 90 degrees vertical distance from the sun. UV-, green- and red-filters have been used. The results showed a diminution of the intensity during the eclipse of about 3 powers of ten. The sky brightness in the point 90 degrees distant during the total eclipse was similar to the brightness when sun is 7 degrees below the horizon. About one minute before the total eclipse the degree of polarization diminuished to zero. — Furthermore photos of nearly the total sky were made using two cameras with wide angle lenses.

PhysicsBrightnessbusiness.industrySolar eclipsemedia_common.quotation_subjectDiffuse sky radiationVertical distanceAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsPolarization (waves)GeophysicsOpticsGeochemistry and PetrologySkyAstrophysics::Solar and Stellar AstrophysicsDegree of polarizationAstrophysics::Earth and Planetary AstrophysicsbusinessAstrophysics::Galaxy Astrophysicsmedia_commonGeofisica Pura e Applicata
researchProduct