Search results for "shift"

showing 10 items of 1226 documents

Stimulated Emission in InGaN/GaN Multiple Quantum Wells with Different Indium Content

2005

1. IntroductionLight-emitting and laser diodes for the green to near-UV region are basedon quantum structures with the InGaN active region [1]. The indium contentin the wells is a technological parameter that provides a straightforward accessfor the change in the color of the light-emitting device. However, the redshift ofthe emission peak with increase in indium content is caused not only by a simplealloying, but also by carrier localization due to difierence in In and Ga atomic

Physicsbusiness.industryMultiple quantumGeneral Physics and Astronomychemistry.chemical_elementLaserRedshiftlaw.inventionchemistrylawContent (measure theory)OptoelectronicsStimulated emissionbusinessQuantumIndiumDiodeActa Physica Polonica A
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Rotational Doppler Frequency Shift from Time‐Evolving High‐Order Pancharatnam–Berry Phase: A Metasurface Approach

2021

The Doppler frequency shift of sound or electromagnetic waves has been widely investigated in many different contexts and, nowadays, represents a formidable tool in medicine, engineering, astrophysics, and optics. Such effect is commonly described in the framework of the universal energy-momentum conservation law. In particular, the rotational Doppler effect has been recently demonstrated using light carrying orbital angular momentum. When a wave undergoes a cyclic adiabatic transformation of its Hamiltonian, it is known to acquire the so-called Pancharatnam–Berry (PB) phase. In this work, an experimental evidence of the direct connection between the high-order PB phase time evolution on th…

Physicsbusiness.industryPancharatnam–Berry phaseCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsMetasurfacesOpticsGeometric phaseorbital angular momentumDoppler frequencyrotational Doppler frequency shiftHigh orderbusinessLaser & Photonics Reviews
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Soliton pairs in a fiber laser: From anomalous to normal average dispersion regime

2003

We report the observation of self phase-locked pulse pairs in a stretched-pulse fiber laser operating in the normal path-averaged dispersion regime. Numerical simulations agree with our experimental results. More insight is provided with a numerical comparison between intracavity profiles of pulse pairs in anomalous and in normal dispersion regimes. © 2003 Optical Society of America.

Physicsbusiness.industryPhysics::OpticsSoliton (optics)LaserAtomic and Molecular Physics and Opticslaw.inventionPulse (physics)OpticsMode-lockinglawFiber laserDispersion (optics)Dispersion-shifted fiberbusinessBandwidth-limited pulse
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Buildup of terahertz vector dark-soliton trains from induced modulation instability in highly birefringent optical fiber.

2007

We present the experimental observation of generation of vector dark-soliton pulse trains with terahertz repetition rates in the normal dispersion regime of an optical fiber. The polarization solitons build up from induced cross-phase modulation instability of two orthogonal pumps in a highly birefringent fiber.

Physicsbusiness.industrySingle-mode optical fiberPhysics::OpticsPolarization-maintaining optical fiberMicrostructured optical fiberGraded-index fiberAtomic and Molecular Physics and OpticsOpticsZero-dispersion wavelengthOptoelectronicsDispersion-shifted fiberPlastic optical fiberbusinessPhotonic-crystal fiberOptics letters
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Corrections to “Light Modulation Based on Fiber Cladding Mode Coupling Between Concatenated Long-Period Gratings” [Feb 1 152-154]

2011

In the above paper (ibid., vol. 23, no. 3, pp. 152-154, Feb. 1, 2011), there is an error in the eighth line of the abstract. The correct sentence is presented here.

Physicsbusiness.industrySingle-mode optical fiberPolarization-maintaining optical fiberLong-period fiber gratingCladding modeGraded-index fiberAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsOpticsFiber Bragg gratingDispersion-shifted fiberElectrical and Electronic EngineeringPlastic optical fiberbusinessIEEE Photonics Technology Letters
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Radio Observations of the Hubble Deep Field South Region IV: Optical Properties of the Faint Radio Population

2008

The Australia Telescope Hubble Deep Field-South (ATHDFS) survey of the Hubble Deep Field South reaches sensitivities of ~10 miceoJyJy at 1.4, 2.5, 5.2 and 8.7 GHz, making the ATHDFS one of the deepest surveys ever performed with the Australia Telescope Compact Array. Here we present the optical identifications of the ATHDFS radio sources using data from the literature. We find that ~66% of the radio sources have optical counterparts to I = 23.5 mag. Deep HST imaging of the area identifies a further 12% of radio sources. We present new spectroscopic observations for 98 of the radio sources, and supplement these spectroscopic redshifts with photometric ones calculated from 5-band optical imag…

Physicseducation.field_of_studyAstrophysics::High Energy Astrophysical PhenomenaPopulationAstrophysics (astro-ph)Hubble Deep Field SouthAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxyRedshiftLuminositylaw.inventionTelescopeOptical imagingSpace and Planetary SciencelaweducationCaltech Library ServicesAstrophysics::Galaxy Astrophysics
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High redshift galaxies in the ALHAMBRA survey

2015

Context. Most observational results on the high redshift restframe UV-bright galaxies are based on samples pinpointed using the so called dropout technique or Ly-alpha selection. However, the availability of multifilter data allows now replacing the dropout selections by direct methods based on photometric redshifts. In this paper we present the methodology to select and study the population of high redshift galaxies in the ALHAMBRA survey data. Aims. Our aim is to develop a less biased methodology than the traditional dropout technique to study the high redshift galaxies in ALHAMBRA and other multifilter data. Thanks to the wide area ALHAMBRA covers, we especially aim at contributing in th…

Physicseducation.field_of_studyPopulationFOS: Physical sciencesSampling (statistics)Astronomy and AstrophysicsContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesRedshiftGalaxySpace and Planetary ScienceLimiting magnitudeAstrophysics of Galaxies (astro-ph.GA)Probability distributioneducationAstrophysics::Galaxy AstrophysicsPhotometric redshiftAstronomy & Astrophysics
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RELIABILITY OF THE DETECTION OF THE BARYON ACOUSTIC PEAK

2008

The correlation function of the distribution of matter in the universe shows, at large scales, baryon acoustic oscillations, which were imprinted prior to recombination. This feature was first detected in the correlation function of the luminous red galaxies (LRG) of the Sloan Digital Sky Survey (SDSS). The final release (DR7) of the SDSS has been recently made available, and the useful volume is about two times bigger than in the old sample. We present here, for the first time, the redshift space correlation function of this sample at large scales together with that for one shallower, but denser volume-limited subsample drawn from the 2dF redshift survey. We test the reliability of the det…

Physicsmedia_common.quotation_subjectAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCorrelation function (astronomy)AstrophysicsRedshift surveyGalaxyRedshiftBaryonDistribution (mathematics)Space and Planetary ScienceSkyBaryon acoustic oscillationsAstrophysics::Galaxy Astrophysicsmedia_commonThe Astrophysical Journal
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XMM-Newton First-Light Observations of the Hickson Galaxy Group 16

2000

This paper presents the XMM-Newton first-light observations of the Hickson-16 compact group of galaxies. Groups are possibly the oldest large-scale structures in the Universe, pre-dating clusters of galaxies, and are highly evolved. This group of small galaxies, at a redshift of 0.0132 (or 80 Mpc) is exceptional in the having the highest concentration of starburst or AGN activity in the nearby Universe. So it is a veritable laboratory for the study of the relationship between galaxy interactions and nuclear activity. Previous optical emission line studies indicated a strong ionising continuum in the galaxies, but its origin, whether from starbursts, or AGN, was unclear. Combined imaging and…

Physicsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Continuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsGalaxies: activeAstrophysicsFirst lightAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy mergerAstrophysicsGalaxyUniverseRedshiftCompact groupSpace and Planetary ScienceGalaxy groupGalaxies: starburstX-rays: galaxieAstrophysics::Galaxy Astrophysicsmedia_common
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Optical pumping and unstable nuclei

1985

The paper reviews the application of optical pumping to short-lived nuclei, where either the nuclear polarisation is detected by the β-decay asymmetry or the atomic polarisation by Stern-Gerlach-analyzer. Moreover the paper deals with collinear laser spectroscopy on beams of short-lived, mass-separated isotopes. The aim of the experiments is the systematic investigation of nuclear structure through the determination of spin, moments and charge radii from the hyperfine structure and isotopic shift of the atomic spectra. The impact of these experiments on the theory of nuclear forces and structure is discussed by means of a few examples.

Physicsmedia_common.quotation_subjectNuclear structureGeneral Physics and AstronomyAsymmetryOptical pumpingIsotopic shiftNuclear forcePhysics::Atomic PhysicsAtomic physicsNuclear ExperimentSpin (physics)SpectroscopyHyperfine structuremedia_commonAnnales de Physique
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