Search results for "Computational physics"

showing 10 items of 725 documents

Performance potential for simulating spin models on GPU

2012

Graphics processing units (GPUs) are recently being used to an increasing degree for general computational purposes. This development is motivated by their theoretical peak performance, which significantly exceeds that of broadly available CPUs. For practical purposes, however, it is far from clear how much of this theoretical performance can be realized in actual scientific applications. As is discussed here for the case of studying classical spin models of statistical mechanics by Monte Carlo simulations, only an explicit tailoring of the involved algorithms to the specific architecture under consideration allows to harvest the computational power of GPU systems. A number of examples, ran…

Spin glassPhysics and Astronomy (miscellaneous)Computer scienceMonte Carlo methodFOS: Physical sciencesComputational scienceCUDAHigh Energy Physics - LatticeStatistical physicsGraphicsCondensed Matter - Statistical MechanicsNumerical AnalysisStatistical Mechanics (cond-mat.stat-mech)Applied MathematicsHigh Energy Physics - Lattice (hep-lat)RangingStatistical mechanicsDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksComputational Physics (physics.comp-ph)Computer Science ApplicationsComputational MathematicsModeling and SimulationIsing modelParallel temperingPhysics - Computational Physics
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Efficient polarization of high-angular-momentum systems

2016

We propose methods of optical pumping that are applicable to open, high-angular-momentum transitions in atoms and molecules, for which conventional optical pumping would lead to significant population loss. Instead of applying circularly polarized cw light, as in conventional optical pumping, we propose to use techniques for coherent population transfer (e.g., adiabatic fast passage) to arrange the atoms so as to increase the entropy removed from the system with each spontaneous decay from the upper state. This minimizes the number of spontaneous-emission events required to produce a stretched state, thus reducing the population loss due to decay to other states. To produce a stretched stat…

Spontaneous decayPhysicsAngular momentumeducation.field_of_studyPhotonAtomic Physics (physics.atom-ph)Atoms in moleculesPopulationPhysics::OpticsFOS: Physical sciencesQuantum number01 natural sciencesphysics.atom-phPhysics - Atomic PhysicsComputational physics010309 opticsOptical pumpingDark stateTotal angular momentum quantum numberAtom0103 physical sciencesAtomic physics010306 general physicsAdiabatic processeducation
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Simulating spin models on GPU

2010

Over the last couple of years it has been realized that the vast computational power of graphics processing units (GPUs) could be harvested for purposes other than the video game industry. This power, which at least nominally exceeds that of current CPUs by large factors, results from the relative simplicity of the GPU architectures as compared to CPUs, combined with a large number of parallel processing units on a single chip. To benefit from this setup for general computing purposes, the problems at hand need to be prepared in a way to profit from the inherent parallelism and hierarchical structure of memory accesses. In this contribution I discuss the performance potential for simulating…

Statistical Mechanics (cond-mat.stat-mech)Computer scienceHigh Energy Physics - Lattice (hep-lat)Monte Carlo methodFOS: Physical sciencesGeneral Physics and AstronomyParallel computingComputational Physics (physics.comp-ph)Power (physics)CUDAHigh Energy Physics - LatticeParallel processing (DSP implementation)Hardware and ArchitectureParallelism (grammar)Ising modelGraphicsPhysics - Computational PhysicsVideo gameCondensed Matter - Statistical MechanicsComputer Physics Communications
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Physically-inspired computational tools for sharp detection of material inhomogeneities in magnetic imaging

2019

Detection of material inhomogeneities is an important task in magnetic imaging and plays a significant role in understanding physical processes. For example, in spintronics, the sample heterogeneity determines the onset of current-driven magnetization motion. While often a significant effort is made in enhancing the resolution of an experimental technique to obtain a deeper insight into the physical properties, here we want to emphasize that an advantageous data analysis has the potential to provide a lot more insight into given data set, in particular when being close to the resolution limit where the noise becomes at least of the same order as the signal. In this work, we introduce two to…

Statistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesComputational Physics (physics.comp-ph)Physics - Computational PhysicsCondensed Matter - Statistical Mechanics
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TheINTEGRALspectrometer SPI: performance of point-source data analysis

2005

The performance of the SPI point-source data analysis system is assessed using a combination of simulations and of observations gathered during the first year of INTEGRAL operations. External error estimates are derived by comparing source positions and fluxes obtained from independent analyses. When the source detection significance provided by the SPIROS imaging reconstruction program increases from ∼10 to ∼100, the errors decrease as the inverse of the detection significance, with values from ∼10 to ∼1 arcmin in positions, and from ∼10 to ∼1 per cent in relative flux. These errors are dominated by Poisson counting noise. Our error estimates are consistent with those provided by the SPIRO…

Statistical noisePoint sourceInstrumentationdata analysis -gamma raysPoisson distribution01 natural sciencesNoise (electronics)[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols.namesakeSignal-to-noise ratioOptics0103 physical sciencesSpurious relationship010303 astronomy & astrophysicsinstrumentationPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryAstronomy and AstrophysicsComputational physicsobservationsSpace and Planetary SciencesymbolsDeconvolutionbusinessmiscellaneous -methodsMonthly Notices of the Royal Astronomical Society
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Quantitative analysis of numerical estimates for the permeability of porous media from lattice-Boltzmann simulations

2010

During the last decade, lattice-Boltzmann (LB) simulations have been improved to become an efficient tool for determining the permeability of porous media samples. However, well known improvements of the original algorithm are often not implemented. These include for example multirelaxation time schemes or improved boundary conditions, as well as different possibilities to impose a pressure gradient. This paper shows that a significant difference of the calculated permeabilities can be found unless one uses a carefully selected setup. We present a detailed discussion of possible simulation setups and quantitative studies of the influence of simulation parameters. We illustrate our results b…

Statistics and ProbabilityMaterials scienceSignificant differenceFluid Dynamics (physics.flu-dyn)Lattice Boltzmann methodsFOS: Physical sciencesStatistical and Nonlinear PhysicsPhysics - Fluid DynamicsMechanicsComputational Physics (physics.comp-ph)Permeability (earth sciences)Permeability measurementsBoundary value problemStatistics Probability and UncertaintyPorous mediumPhysics - Computational PhysicsPressure gradient
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Noise-induced resonance-like phenomena in InP crystals embedded in fluctuating electric fields

2016

We explore and discuss the complex electron dynamics inside a low-doped n-type InP bulk embedded in a sub-THz electric field, fluctuating for the superimposition of an external source of Gaussian correlated noise. The results presented in this study derive from numerical simulations obtained by means of a multi-valley Monte Carlo approach to simulate the nonlinear transport of electrons inside the semiconductor crystal. The electronic noise characteristics are statistically investigated by calculating the correlation function of the velocity fluctuations, its spectral density and the integrated spectral density, i.e. the total noise power, for different values of both amplitude and frequenc…

Statistics and ProbabilityNoise powerField (physics)02 engineering and technologyElectron01 natural sciencesNoise (electronics)Settore FIS/03 - Fisica Della MateriaBoltzmann equationsymbols.namesakeCorrelation functionElectric fieldQuantum mechanics0103 physical sciencesstochastic particle dynamics (theory)010306 general physicsfluctuations (theory)Physicstransport properties (theory)Statistical and Nonlinear Physics021001 nanoscience & nanotechnologySettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Computational physicsAmplitudeGaussian noisesymbolsStatistics Probability and Uncertainty0210 nano-technologyJournal of Statistical Mechanics: Theory and Experiment
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The influence of noise on electron dynamics in semiconductors driven by a periodic electric field

2009

Studies about the constructive aspects of noise and fluctuations in different non-linear systems have shown that the addition of external noise to systems with an intrinsic noise may result in a less noisy response. Recently, the possibility to reduce the diffusion noise in semiconductor bulk materials by adding a random fluctuating contribution to the driving static electric field has been tested. The present work extends the previous theories by considering the noise-induced effects on the electron transport dynamics in low-doped n-type GaAs samples driven by a high-frequency periodic electric field (cyclostationary conditions). By means of Monte Carlo simulations, we calculate the change…

Statistics and ProbabilityNoise powerMaterials scienceField (physics)Cyclostationary processElectric fieldMonte Carlo methodSpectral densityStatistical and Nonlinear PhysicsElectronStatistics Probability and UncertaintyNoise (electronics)Computational physicsJournal of Statistical Mechanics: Theory and Experiment
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WENO schemes applied to the quasi-relativistic Vlasov-Maxwell model for laser-plasma interaction

2014

Abstract In this paper we focus on WENO-based methods for the simulation of the 1D Quasi-Relativistic Vlasov–Maxwell (QRVM) model used to describe how a laser wave interacts with and heats a plasma by penetrating into it. We propose several non-oscillatory methods based on either Runge–Kutta (explicit) or Time-Splitting (implicit) time discretizations. We then show preliminary numerical experiments.

Strategy and ManagementFOS: Physical sciences010103 numerical & computational mathematics01 natural scienceslaw.inventionMathematics::Numerical Analysislaser-plasma interactionMathematics - Analysis of PDEslawMedia TechnologyFOS: MathematicsVlasov--Maxwell[MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP]General Materials ScienceMathematics - Numerical Analysis0101 mathematicsMarketingPhysicsPhysics::Computational PhysicsWENOPlasmaNumerical Analysis (math.NA)Computational Physics (physics.comp-ph)LaserRunge--Kutta schemes010101 applied mathematicsClassical mechanicsStrang splittingFocus (optics)Physics - Computational PhysicsAnalysis of PDEs (math.AP)Strang splitting
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3D MHD MODELING of TWISTED CORONAL LOOPS

2016

We perform MHD modeling of a single bright coronal loop to include the interaction with a non-uniform magnetic field. The field is stressed by random footpoint rotation in the central region and its energy is dissipated into heating by growing currents through anomalous magnetic diffusivity that switches on in the corona above a current density threshold. We model an entire single magnetic flux tube, in the solar atmosphere extending from the high-beta chromosphere to the low-beta corona through the steep transition region. The magnetic field expands from the chromosphere to the corona. The maximum resolution is ~30 km. We obtain an overall evolution typical of loop models and realistic loo…

Sun: activity; Sun: corona; Astronomy and Astrophysics; Space and Planetary Science010504 meteorology & atmospheric sciencescorona [Sun]Astrophysics::High Energy Astrophysical PhenomenaNDASFOS: Physical sciences01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaSun: activity0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsQB Astronomyactivity [Sun]010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesQBPhysicsFlux tubeSun: coronaAstronomy and AstrophysicsCoronal loopCoronaMagnetic fluxComputational physicsMagnetic fieldQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsMagnetic diffusivity
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