Search results for "Wavelength"

showing 10 items of 741 documents

Effective temperature and scaling laws of polarized quantum vortex bundles

2011

Abstract An effective non-equilibrium temperature is defined for (locally) polarized and dense turbulent superfluid vortex bundles, related to the average energy of the excitations (Kelvin waves) of vortex lines. In the quadratic approximation of the excitation energy in terms of the wave amplitude A, a previously known scaling relation between amplitude and wavelength k of Kelvin waves in polarized bundles, namely A ∝ k − 1 / 2 , follows from the homogeneity of the effective temperature. This result is analogous to that of the well-known equipartition result in equilibrium systems.

PhysicsCondensed matter physicsNon-equilibrium temperature Turbulent superfluids Vortices Scaling laws Non-equilibrium thermodynamicsQuantum vortexGeneral Physics and AstronomyNon-equilibrium thermodynamicsVortexsymbols.namesakeWavelengthAmplitudesymbolsKelvin waveScalingSettore MAT/07 - Fisica MatematicaEquipartition theorem
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Surface-acoustic-wave-induced space-charge waves in electron–hole systems

2005

Abstract Space-charge waves in an electron–hole system are studied, which are excited by a moving grating provided by a surface acoustic wave (SAW). The SAW induces a constant current that may change its sign, when a constant electric field is applied opposite to the wave propagation direction. Current resonances are predicted to appear, when the SAW wavelength and frequency match the ones of the space-charge wave.

PhysicsCondensed matter physicsWave propagationbusiness.industrySurface acoustic waveGeneral ChemistryCondensed Matter PhysicsWavelengthsymbols.namesakeOpticsSurface waveWave shoalingMaterials ChemistrysymbolsRayleigh wavebusinessMechanical waveLongitudinal waveSolid State Communications
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Vortex solitons in photonic crystal fibers

2003

We demonstrate the existence of vortex soliton solutions in photonic crystal fibers. We analyze the role played by the photonic crystal fiber defect in the generation of optical vortices. An analytical prediction for the angular dependence of the amplitude and phase of the vortex solution based on group theory is also provided. Furthermore, all the analysis is performed in the non-paraxial regime.

PhysicsCondensed matter physicsbusiness.industryPhase (waves)Physics::OpticsFOS: Physical sciencesSoliton (optics)Microstructured optical fiberPattern Formation and Solitons (nlin.PS)Nonlinear Sciences - Pattern Formation and SolitonsAtomic and Molecular Physics and OpticsVortexZero-dispersion wavelengthOpticsCondensed Matter::SuperconductivitybusinessOptical vortexPhotonic crystalPhotonic-crystal fiber
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Structure of the Accretion Disk in the Lensed Quasar Q2237+0305 from Multi-Epoch and Multi-Wavelength Narrow Band Photometry

2015

We present estimates for the size and the logarithmic slope of the disk temperature profile of the lensed quasar Q2237+0305, independent of the component velocities. These estimates are based on six epochs of multi-wavelength narrowband images from the Nordic Optical Telescope. For each pair of lensed images and each photometric band, we determine the microlensing amplitude and chromaticity using pre-existing mid-IR photometry to define the baseline for no microlensing magnification. A statistical comparison of the combined microlensing data (6 epochs $\times$ 5 narrow bands $\times$ 6 image pairs) with simulations based on microlensing magnification maps gives Bayesian estimates for the ha…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstronomy and AstrophysicsQuasarMulti wavelengthAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencesAccretion (astrophysics)NarrowbandAccretion discSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics0105 earth and related environmental sciences
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A Study of Gravitational Lens Chromaticity with the Hubble Space Telescope

2011

We report Hubble Space Telescope observations of 6 gravitational lenses with the Advanced Camera for Surveys. We measured the flux ratios between the lensed images in 6 filters from 8140\AA\ to 2200\AA. In 3 of the systems, HE0512$-$3329, B1600+434, and H1413+117, we were able to construct UV extinction curves partially overlapping the 2175\AA\ feature and characterize the properties of the dust relative to the Galaxy and the Magellanic Clouds. In HE1104$-$1804 we detect chromatic microlensing and use it to study the physical properties of the quasar accretion disk. For a Gaussian model of the disk $\exp(-r^2/2 r_s^2)$, scaling with wavelength as $r_s \propto \lambda^p$, we estimate $r_s(\l…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Extinction (astronomy)FOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational microlensing01 natural sciencesAdvanced Camera for SurveysGalaxyGravitationWavelengthGravitational lens13. Climate actionSpace and Planetary Science0103 physical sciences010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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VLBI imaging of M81* at 43GHz

2011

The nearby spiral galaxy M81 harbors in its core a Low-Luminosity AGN (LLAGN), and appears closely related to the more distant and powerful AGNs seen in quasars and radio galaxies. The intrinsic size of this object is unknown due to scattering, and it has shown a core-jet morphology with weak extended emission rotating with wavelength. The proximity of M\,81 (D=3.63 Mpc) allows a detailed investigation of its nucleus to be made. The nucleus is four orders of magnitude more luminous than the Galactic centre, and is therefore considered a link between SgrA* and the more powerful nuclei of radio galaxies and quasars. Our main goal was to determine the size of M81* at a shorter wavelength thus …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Spiral galaxyRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPosition angleWavelengthSpace and Planetary ScienceAngular diameterVery-long-baseline interferometryVery Long Baseline ArrayAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Exact reconstruction of thz sub-λ source features in knife-edge measurements

2013

The spatial features of a sub-wavelength terahertz source are not accessible using time-integrated knife-edge techniques due to the non-separable space-time nature of the radiated field and to systematic modifications induced by the blade itself. We show that combining knife-edge with a time resolved electro-optical sampling, the space-time coupling can be addressed and the source field profile can be exactly reconstructed.

PhysicsCouplingPhase-sensitive field characterizationBlade (geometry)Terahertz radiationbusiness.industrySettore ING-INF/02 - Campi ElettromagneticiEdge (geometry)Lambdasubwavelength sourceSettore ING-INF/01 - ElettronicaSource fieldAtomic and Molecular Physics and OpticsOpticsSampling (signal processing)subwavelength sourcesspatiotemporal field characterizationElectrical and Electronic EngineeringTime-resolved spectroscopybusinessterahertz (THz) sources
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Impact of the scattering coefficient of scintillation crystals (LYSO and LSO) on depth of interaction resolution

2008

Intrinsic parameters in scintillation crystals play a crucial role in the measured spatial and energy resolutions. In many cases the measurement of these intrinsic parameters is difficult to be carried out or even there are parameters that need a specific setup to be measured directly, e.g. the intrinsic light yield and the absorption and scattering coefficients. These uncertainties in the parametrization of the characteristics of the scintillation crystals make it quite difficult to evaluate the quality and characteristics of the scintillation crystals and their impact on the resolutions. Results of measurements of depth of interaction and its resolutions for three different scintillation …

PhysicsCrystalWavelengthOpticsScatteringbusiness.industryTransmittancebusinessAbsorption (electromagnetic radiation)Refractive indexLight scatteringLyso-2008 IEEE Nuclear Science Symposium Conference Record
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Optical demultiplexing of millimeter-wave subcarriers for wireless channel distribution employing dual wavelength FBGs

2007

An optical mm-wave demultiplexer is presented. Double sideband modulation with suppressed optical carrier and filtering properties of dual overwritten fiber Bragg gratings are the fundamentals for optical demultiplexing of mm-wave radio-on-fiber signals: using a single optical carrier, Millimeter-wave signals of 20 and 40 GHz frequencies carrying independent data are created, transmitted over fiber, demultiplexed and wireless distributed to be detected and data recovered in a mobile unit. Double sideband modulation with suppressed optical carrier yields no power penalty due to chromatic dispersion, while the filtering properties of the dual overwritten fiber Bragg gratings allow less than −…

PhysicsDemultiplexerbusiness.industryOptical communicationPhysics::OpticsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsOpticsFiber Bragg gratingOptical Carrier transmission ratesWavelength-division multiplexingDouble-sideband suppressed-carrier transmissionElectrical and Electronic EngineeringPhysical and Theoretical ChemistryPlastic optical fiberbusinessOptical aberrationOptics Communications
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Subwavelength sound screening by coupling space-coiled Fabry-Perot resonators

2017

We explore broadband and omnidirectional low frequency sound screening based on locally resonant acoustic metamaterials. We show that the coupling of different resonant modes supported by Fabry-Perot cavities can efficiently generate asymmetric lineshapes in the transmission spectrum, leading to a broadband sound opacity. The Fabry-Perot cavities are space-coiled in order to shift the resonant modes under the diffraction edge, which guaranty the opacity band for all incident angles. Indeed, the deep subwavelength feature of the cavities leads to avoid diffraction that have been proved to be the main limitation of omnidirectional capabilities of locally resonant perforated plates. We experim…

PhysicsDiffractionOpacitybusiness.industryAttenuationGeneral Physics and AstronomyMetamaterialPhysics::OpticsFOS: Physical sciencesPhysics - Applied Physics02 engineering and technologyAcoustic waveApplied Physics (physics.app-ph)021001 nanoscience & nanotechnology01 natural sciencesResonatorWavelengthOptics0103 physical sciences010306 general physics0210 nano-technologybusinessFabry–Pérot interferometer
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