Search results for "LONG"

showing 10 items of 3969 documents

Thermal rippling behavior of graphane

2012

Thermal fluctuations of single layer hydrogenated graphene (graphane) are investigated using large scale atomistic simulations. By analyzing the mean square value of the height fluctuations $$ and the height-height correlation function $H(q)$ for different system sizes and temperatures we show that hydrogenated graphene is an un-rippled system in contrast to graphene. The height fluctuations are bounded, which is confirmed by a $ H(q) $ tending to a constant in the long wavelength limit instead of showing the characteristic scaling law $ q^{4-\eta} (\eta \simeq 0.85)$ predicted by membrane theory. This unexpected behaviour persists up to temperatures of at least 900 K and is a consequence o…

PhysicsCondensed Matter - Materials ScienceCondensed matter physicsLong wavelength limitGraphenePhysicsMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesThermal fluctuationsNanotechnologyBendingCondensed Matter PhysicsElectronic Optical and Magnetic Materialslaw.inventionchemistry.chemical_compoundMolecular geometrychemistryCorrelation functionlawThermalGraphanePhysical review : B : condensed matter and materials physics
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Positron Annihilation in Steel Samples Deformed by Uniaxial Tension

2008

Angular distributions of the positron annihilation quanta were measured for steel ST2 SAL samples deformed by uniaxial tension up to difierent deformation degrees. The dependences of the S parameter on the relative elongation of the samples are presented. The positron annihilation data for steel are compared with the results obtained previously for polycrystalline iron samples deformed by uniaxial tension up to difierent deformation degrees in the proportionality and limited proportionality regions.

PhysicsCondensed matter physicsUniaxial tensionGeneral Physics and AstronomyCrystalliteDeformation (meteorology)ElongationPhysics::Classical PhysicsPositron annihilationActa Physica Polonica A
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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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LONG-TERM MONITORING, TIME DELAY, AND MICROLENSING IN THE GRAVITATIONAL LENS SYSTEM Q0142-100

2013

We present twelve years of monitoring of the gravitational lens Q0142-100 from the Teide Observatory. The data, taken from 1999 to 2010, comprise 105 observing nights with the IAC80 telescope. The application of the delta2-method to the dataset leads to a value of the time delay between both components of the system of 72+/-22 days (68 per cent confidence level), consistent within the uncertainties with the latest previous results. With this value in mind a possible microlensing event is detected in Q0142-100.

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Event (relativity)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGravitational microlensinglaw.inventionTelescopeGravitational lensSpace and Planetary ScienceObservatorylawLong term monitoringAstrophysics - Cosmology and Nongalactic AstrophysicsThe Astrophysical Journal
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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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Mechanically Based Nonlocal Euler-Bernoulli Beam Model

2014

AbstractThis paper presents a nonlocal Euler-Bernoulli beam model. It is assumed that the equilibrium of a beam segment is attained because of the classical local stress resultants, along with long-range volume forces and moments exchanged by the beam segment with all the nonadjacent beam segments. Elastic long-range volume forces/moments are considered, built as linearly depending on the product of the volumes of the interacting beam segments and on generalized measures of their relative motion, based on the pure deformation modes of the beam. Attenuation functions governing the space decay of the nonlocal effects are introduced. The motion equations are derived in an integro-differential …

PhysicsDeformation (mechanics)Mechanical EngineeringAttenuationEquations of motionSpace (mathematics)VibrationLong-range interactionClassical mechanicsNonlocal elasticityEuler-Bernoulli beamStress resultantsPhysics::Accelerator PhysicsFree vibrationsSettore ICAR/08 - Scienza Delle CostruzioniStaticsStaticBeam (structure)
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Coherence loss in phase-referenced VLBI observations

2010

Context. Phase-referencing is a standard calibration technique in radio interferometry, particularly suited for the detection of weak sources close to the sensitivity limits of the interferometers. However, effects from a changing atmosphere and inaccuracies in the correlator model may affect the phase-referenced images, and lead to wrong estimates of source flux densities and positions. A systematic observational study of signal decoherence in phase-referencing and its effects in the image plane has not been performed yet. Aims. We systematically studied how the signal coherence in Very-Long-Baseline-Interferometry (VLBI) observations is affected by a phase-reference calibration at differe…

PhysicsDynamic rangePhase (waves)Astrophysics::Instrumentation and Methods for AstrophysicsFluxAstronomy and AstrophysicsContext (language use)interferometers [Instrumentation]AstrophysicsAtmospheric effectsComputational physicsTechniques : interferometric; Atmospheric effects; Instrumentation : interferometersInterferometrySpace and Planetary ScienceVery-long-baseline interferometrySource separationinterferometric [Techniques]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]Coherence (physics)
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15 years of very long baseline interferometry observations of two compact radio sources in Messier 82

2006

We present the results of a second epoch of 18cm global Very Long-Baseline Interferometry (VLBI) observations, taken on 23 February 2001, of the central kiloparsec of the nearby starburst galaxy Messier 82. These observations further investigate the structural and flux evolution of the most compact radio sources in the central region of M82. The two most compact radio objects in M82 have been investigated (41.95+575 and 43.31+592). Using this recent epoch of data in comparison with our previous global VLBI observations and two earlier epochs of European VLBI Network observations we measure expansion velocities in the range of 1500-2000km/s for 41.95+575, and 9000-11000km/s for 43.31+592 usi…

PhysicsEuropean VLBI NetworkEpoch (reference date)FluxAstronomy and AstrophysicsAstrophysicsMessier objectGalaxySupernovasymbols.namesakeInterferometrySpace and Planetary ScienceVery-long-baseline interferometrysymbolsMonthly Notices of the Royal Astronomical Society
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Expansion of SN 1993J: New λλ6 and 13 cm images

1997

Abstract Radio supernovae are rare events among supernovae, usually taking place in distant galaxies. In recent years, great progress has been made in the study of radio supernovae with high angular resolution, due to advances in the VLBI technique and to the lucky occurrence of the powerful supernova SN 1993J in M81 only 3.6 Mpc distant. Its spatial structure has been unveiled and its expansion rate determined at 3.6 cm. Here we present new preliminary VLBI results on the expansion of this supernova at 6 and 13 cm. We resolve the shell at both wavelengths. The size estimates at 6 cm indicate a lower expansion rate than previously estimated. This may be the first evidence of deceleration.

PhysicsExpansion rateSpatial structureAstrophysics::High Energy Astrophysical PhenomenaAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxySupernovaWavelengthVery-long-baseline interferometryAstrophysics::Solar and Stellar AstrophysicsAngular resolutionAstrophysics::Galaxy AstrophysicsVistas in Astronomy
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The finite element method for fractional non-local thermal energy transfer in non-homogeneous rigid conductors

2015

Abstract In a non-local fractional-order model of thermal energy transport recently introduced by the authors, it is assumed that local and non-local contributions coexist at a given observation scale: while the first is described by the classical Fourier transport law, the second involves couples of adjacent and non-adjacent elementary volumes, and is taken as proportional to the product of the masses of the interacting volumes and their relative temperature, through a material-dependent, distance-decaying power-law function. As a result, a fractional-order heat conduction equation is derived. This paper presents a pertinent finite element method for the solution of the proposed fractional…

PhysicsFinite element methodNumerical Analysisbusiness.industryApplied MathematicsMathematical analysisFinite differenceFinite element method; Fractional calculus; Long-range heat transport; Non-homogeneous conductors; Modeling and Simulation; Numerical Analysis; Applied MathematicsMixed finite element methodFractional calculuFinite element methodFractional calculussymbols.namesakeLong-range heat transportFourier transformModeling and SimulationsymbolsHeat equationNon-homogeneous conductorbusinessSettore ICAR/08 - Scienza Delle CostruzioniNumerical AnalysiThermal energyExtended finite element method
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