Search results for "Computational physics"

showing 10 items of 725 documents

CHANGES OF ELECTRONIC NOISE INDUCED BY OSCILLATING FIELDS IN BULK GaAs SEMICONDUCTORS

2008

A Monte Carlo study of hot-electron intrinsic noise in a n-type GaAs bulk driven by one or two mixed cyclostationary electric fields is presented. The noise properties are investigated by computing the spectral density of velocity fluctuations. An analysis of the noise features as a function of the amplitudes and frequencies of two applied fields is presented. Numerical results show that it is possible to reduce the intrinsic noise. The best conditions to realize this effect are discussed.

PhysicsElectronic noiseCyclostationary processGeneral MathematicsMonte Carlo methodQuantum noiseShot noiseField-mixing conditionGeneral Physics and AstronomySpectral densityNoise (electronics)Settore FIS/03 - Fisica Della MateriaComputational physicsElectric fieldFlicker noiseStatistical physicsMonte Carlo simulationFluctuation and Noise Letters
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Simple absorbing layer conditions for shallow wave simulations with Smoothed Particle Hydrodynamics

2013

Abstract We study and implement a simple method, based on the Perfectly Matched Layer approach, to treat non reflecting boundary conditions with the Smoothed Particles Hydrodynamics numerical algorithm. The method is based on the concept of physical damping operating on a fictitious layer added to the computational domain. The method works for both 1D and 2D cases, but here we illustrate it in the case of 1D and 2D time dependent shallow waves propagating in a finite domain.

PhysicsEnvironmental EngineeringOcean EngineeringFluid mechanicsMechanicsFluid mechanics Boundary condition Absorbing layer Lagrangian numerical method SPH Shallow water modelDomain (mathematical analysis)Computational physicsSmoothed-particle hydrodynamicsPerfectly matched layerSimple (abstract algebra)Boundary value problemLayer (object-oriented design)Ocean Engineering
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Morphology and Dynamics of Relativistic Jets

1997

We present a comprehensive analysis of the morphology and dynamics of relativistic pressure-matched axisymmetric jets. The numerical simulations have been carried out with a high-resolution shock-capturing hydrocode based on an approximate relativistic Riemann solver derived from the spectral decomposition of the Jacobian matrices of relativistic hydrodynamics. We discuss the dependence of the jet morphology on several parameters, paying special attention to the relativistic effects caused by high Lorentz factors and large internal energies of the beam flow. The parameter space of our analysis is spanned by the ratio of the beam and ambient medium rest mass density (η), the beam Mach number…

PhysicsEquation of state (cosmology)Astrophysics::High Energy Astrophysical PhenomenaElliptic flowAstronomy and AstrophysicsEnergy–momentum relationMechanicsComputational physicsRelativistic particleLorentz factorsymbols.namesakeRelativistic beamingAstrophysical jetSpace and Planetary SciencesymbolsRelativistic quantum chemistryThe Astrophysical Journal
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A multispacecraft analysis of a small-scale transient entrained by solar wind streams

2009

The images taken by the Heliospheric Imagers (HIs), part of the SECCHI imaging package onboard the pair of STEREO spacecraft, provide information on the radial and latitudinal evolution of the plasma compressed inside corotating interaction regions (CIRs). A plasma density wave imaged by the HI instrument onboard STEREO-B was found to propagate towards STEREO-A, enabling a comparison between simultaneous remote-sensing and in situ observations of its structure to be performed. In situ measurements made by STEREO-A show that the plasma density wave is associated with the passage of a CIR. The magnetic field compressed after the CIR stream interface (SI) is found to have a planar distribution…

PhysicsExtraterrestrial Physics Space SciencesOrbital planecoronal mass ejection [Interplanetary medium]PhysicsStellar magnetic fieldAstronomyFluxAstronomy and AstrophysicsPlasmaAstrophysicsMagnetic fieldComputational physicsMeteorology/ClimatologySolar windSpace and Planetary SciencePhysics::Space Physicsmagnetic field [Sun]Astrophysics::Solar and Stellar AstrophysicsHeliospheric current sheetMagnetic cloudAstrophysics::Earth and Planetary Astrophysicscorotating interaction regions [Sun]
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Surface waves in solar granulation observed with {\sc Sunrise}

2010

Solar oscillations are expected to be excited by turbulent flows in the intergranular lanes near the solar surface. Time series recorded by the IMaX instrument aboard the {\sc Sunrise} observatory reveal solar oscillations at high resolution, which allow studying the properties of oscillations with short wavelengths. We analyze two times series with synchronous recordings of Doppler velocity and continuum intensity images with durations of 32\thinspace min and 23\thinspace min, resp., recorded close to the disk center of the Sun to study the propagation and excitation of solar acoustic oscillations. In the Doppler velocity data, both the standing acoustic waves and the short-lived, high-deg…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAcoustic waveComputational physicsStanding waveSuperposition principleWavelengthAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSurface waveSunriseWavenumberAstrophysics::Solar and Stellar AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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Sensitivity to Initial Conditions in an Extended Activator--Inhibitor Model for the Formation of Patterns

2018

Despite simplicity, the synchronous cellular automaton [D.A. Young, Math. Biosci. 72, 51 (1984)] enables reconstructing basic features of patterns of skin. Our extended model allows studying the formatting of patterns and their temporal evolution also on the favourable and hostile environments. As a result, the impact of different types of an environment is accounted for the dynamics of patterns formation. The process is based on two diffusible morphogens, the short-range activator and the long-range inhibitor, produced by differentiated cells (DCs) represented as black pixels. For a neutral environment, the extended model reduces to the original one. However, even the reduced model is stat…

PhysicsFOS: Physical sciencesGeneral Physics and AstronomyComputational Physics (physics.comp-ph)Reduced modelCellular automatonExtended modelAverage sizeInitial distributionFOS: Biological sciencesCell Behavior (q-bio.CB)Quantitative Biology - Cell BehaviorBiological systemPhysics - Computational PhysicsActa Physica Polonica B
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2014

We present a unified framework for the description of the interaction of fast electrons with complex nanostructures based on the Green dyadic method. We show that the computation of a generalized field propagator yields the electron energy losses and cathodoluminescence of nano-objects of arbitrary morphologies embedded in complex dielectric media. Spectra and maps for both penetrating and non-penetrating electron trajectories are provided. This numerical approach can be extended to describe complex experiments involving fast electrons and optically excited nanostructures.

PhysicsField (physics)Electron energy loss spectroscopySurface plasmonPhysics::OpticsGeneral Physics and AstronomyPropagatorCathodoluminescence02 engineering and technologyElectron021001 nanoscience & nanotechnology01 natural sciencesComputational physicsExcited state0103 physical sciencesAtomic physics010306 general physics0210 nano-technologyPlasmonNew Journal of Physics
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Possible gyrotron operation in the “no start current” zone caused by the axial dependence of the phase of the resonator field

2018

It is known that gyrotrons (as well as other electron beam driven microwave and millimeter-wave oscillators) can operate in the regime of either soft or hard self-excitation. In the regime of soft self-excitation, the beam current exceeds its starting value; thus, the oscillations can start to grow from the noise produced by electrons. In the regime of hard self-excitation, the beam current is less than its starting value. Therefore, for exciting the oscillations, a certain start-up scenario is required, which may include the variation of the mod-anode and/or beam voltage or the guiding magnetic field. It was found recently [O. Dumbrajs and G. S. Nusinovich, Phys. Plasmas 25, 013121 (2018)]…

PhysicsField (physics)Phase (waves)ElectronCondensed Matter Physics01 natural sciences010305 fluids & plasmaslaw.inventionComputational physicsMagnetic fieldResonatorlawGyrotron0103 physical sciences010306 general physicsBeam (structure)Noise (radio)Physics of Plasmas
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Magnetic shielding of soft protons in future X-ray telescopes: the case of the ATHENA Wide Field Imager

2018

Both the interplanetary space and the Earth magnetosphere are populated by low energy ($\leq300$ keV) protons that are potentially able to scatter on the reflecting surface of Wolter-I optics of X-ray focusing telescopes and reach the focal plane. This phenomenon, depending on the X-ray instrumentation, can dramatically increase the background level, reducing the sensitivity or, in the most extreme cases, compromising the observation itself. The use of a magnetic diverter, deflecting protons away from the field of view, requires a detailed characterization of their angular and energy distribution when exiting the mirror. We present the first end-to-end Geant4 simulation of proton scattering…

PhysicsField (physics)ProtonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsMagnetosphereFOS: Physical sciencesAstronomy and AstrophysicsX-ray telescopeField of view01 natural sciencesComputational physicsMagnetic field010309 opticsCardinal pointSpace and Planetary Science0103 physical sciencesElectromagnetic shieldinginstrumentation: miscellaneous – telescopesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Monte Carlo Study of Diffusion Noise Reduction in GaAs Operating under Periodic Conditions

2009

The effects of an external correlated source of noise on the intrinsic carrier noise in a low‐doped GaAs bulk, operating under periodic conditions, are investigated. Numerical results confirm that the dynamical response of electrons driven by a high‐frequency periodic electric field receives a benefit by the constructive interplay between the fluctuating field and the intrinsic noise of the system. In particular, in this contribute we show a nonmonotonic behavior of the integrated spectral density, which value critically depends on the correlation time of the external noise source.

PhysicsField (physics)Quantum Monte CarloElectric fieldNoise reductionMonte Carlo methodDynamic Monte Carlo methodStatistical physicsNoise (electronics)Computational physicsMonte Carlo molecular modeling
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