Search results for "Numerical Analysis"

showing 10 items of 883 documents

Many-Body Quantum Dynamics from the Density

2013

We present a local control scheme to construct the external potential v that, for a given initial state, produces a prescribed time-dependent density in an interacting quantum many-body system. This numerical method is efficient and stable even for large and rapid density variations irrespective of the initial state and the interactions. It can at the same time be used to answer fundamental v-representability questions in density functional theory. In particular, in the absence of interactions, it allows us to construct the exact time-dependent Kohn-Sham potential for arbitrary initial states. We illustrate the method in a correlated one-dimensional two-electron system with different intera…

Physics010304 chemical physicsQuantum dynamicsNumerical analysisGeneral Physics and AstronomyConstruct (python library)State (functional analysis)01 natural sciencesAdiabatic theoremScheme (mathematics)0103 physical sciencesDensity functional theoryStatistical physics010306 general physicsQuantum
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Efficient numerical integration of neutrino oscillations in matter

2016

A special purpose solver, based on the Magnus expansion, well suited for the integration of the linear three neutrino oscillations equations in matter is proposed. The computations are speeded up to two orders of magnitude with respect to a general numerical integrator, a fact that could smooth the way for massive numerical integration concomitant with experimental data analyses. Detailed illustrations about numerical procedure and computer time costs are provided.

Physics010308 nuclear & particles physicsComputationNumerical analysisFOS: Physical sciencesNumerical Analysis (math.NA)65L05 65L20Computational Physics (physics.comp-ph)Solver01 natural sciencesNumerical integrationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Classical mechanicsIntegratorMagnus expansion0103 physical sciencesFOS: MathematicsApplied mathematicsMathematics - Numerical Analysis010306 general physicsNeutrino oscillationPhysics - Computational PhysicsNumerical stability
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An algorithm for computing geometric relative velocities through Fermi and observational coordinates

2013

We present a numerical method for computing the \textit{Fermi} and \textit{observational coordinates} of a distant test particle with respect to an observer. We apply this method for computing some previously introduced concepts of relative velocity: \textit{kinematic}, \textit{Fermi}, \textit{spectroscopic} and \textit{astrometric} relative velocities. We also extend these concepts to non-convex normal neighborhoods and we make some convergence tests, studying some fundamental examples in Schwarzschild and Kerr spacetimes. Finally, we show an alternative method for computing the Fermi and astrometric relative velocities.

Physics83C10 83-08 65Z05Physics and Astronomy (miscellaneous)Numerical analysisMathematical analysisRelative velocityFOS: Physical sciencesKinematicsGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)Observer (physics)General Relativity and Quantum CosmologyConvergence testsTest particleSchwarzschild radiusMathematical PhysicsFermi Gamma-ray Space Telescope
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Analytic solutions and Singularity formation for the Peakon b--Family equations

2012

This paper deals with the well-posedness of the b-family equation in analytic function spaces. Using the Abstract Cauchy-Kowalewski theorem we prove that the b-family equation admits, locally in time, a unique analytic solution. Moreover, if the initial data is real analytic and it belongs to H s with s>3/2, and the momentum density u 0-u 0, xx does not change sign, we prove that the solution stays analytic globally in time, for b≥1. Using pseudospectral numerical methods, we study, also, the singularity formation for the b-family equations with the singularity tracking method. This method allows us to follow the process of the singularity formation in the complex plane as the singularity a…

PhysicsAbstract Cauchy-Kowalewski theoremApplied MathematicsNumerical analysisComplex singularitiesNumerical Analysis (math.NA)Spectral analysisFourier spectrumRate of decayPeakonAnalytic solutionMomentumSingularityMathematics - Analysis of PDEsb-family equationFOS: MathematicsSpectral analysis Complex singularities b-family equation Analytic solution Abstract Cauchy-Kowalewski theoremMathematics - Numerical AnalysisComplex planeSettore MAT/07 - Fisica MatematicaMathematical physicsSign (mathematics)Analysis of PDEs (math.AP)
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Sound absorption prediction of linear damped acoustic resonators using a lightweight hybrid model

2019

International audience; A lightweight numerical method is developed to predict the sound absorption coefficient of resonators whose cross-section dimensions are significantly larger compared to the viscous and thermal boundary layer’s thicknesses. This method is based on the boundary layer theory and on the perturbations theory. According to the perturbations theory, in acoustical domains with large dimensions, the fluid viscosity and thermal conductivity only affect the boundary layers. The model proposed in this article combines the lossless Helmholtz wave equation derived from a perfect fluid hypothesis, with viscosity and thermal conductivity values of a real fluid to compute the sound …

PhysicsAcoustics and UltrasonicsComputation efficiencyNumerical analysisAcousticsResonance absorbersDissipationWave equation01 natural sciences7. Clean energy[PHYS.MECA.ACOU]Physics [physics]/Mechanics [physics]/Acoustics [physics.class-ph]010305 fluids & plasmasBoundary layer theoryViscothermal lossesBoundary layersymbols.namesakeViscosityNoise reduction coefficientResonatorHelmholtz free energy0103 physical sciencessymbolsSound absorptionAcoustic modeling010301 acousticsApplied Acoustics
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Numerical Simulations of Jets from Active Galactic Nuclei

2019

Numerical simulations have been playing a crucial role in the understanding of jets from active galactic nuclei (AGN) since the advent of the first theoretical models for the inflation of giant double radio galaxies by continuous injection in the late 1970s. In the almost four decades of numerical jet research, the complexity and physical detail of simulations, based mainly on a hydrodynamical/magneto-hydrodynamical description of the jet plasma, have been increasing with the pace of the advance in theoretical models, computational tools and numerical methods. The present review summarizes the status of the numerical simulations of jets from AGNs, from the formation region in the neighborho…

PhysicsActive galactic nucleus010308 nuclear & particles physicsRadio galaxyplasma physicslcsh:AstronomyNumerical analysisAstrophysics::High Energy Astrophysical PhenomenaTheoretical modelsAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslcsh:QB1-991Astrophysical jetmagneto-hydrodynamics0103 physical sciencesactive galactic nucleinumerical methodsMagnetohydrodynamics010303 astronomy & astrophysicsPhenomenology (particle physics)Astrophysics::Galaxy Astrophysicsrelativistic jetsGalaxies
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Axisymmetric solutions for a chemotaxis model of Multiple Sclerosis

2018

In this paper we study radially symmetric solutions for our recently proposed reaction–diffusion–chemotaxis model of Multiple Sclerosis. Through a weakly nonlinear expansion we classify the bifurcation at the onset and derive the amplitude equations ruling the formation of concentric demyelinating patterns which reproduce the concentric layers observed in Balò sclerosis and in the early phase of Multiple Sclerosis. We present numerical simulations which illustrate and fit the analytical results.

PhysicsApplied MathematicsGeneral MathematicsMultiple sclerosisNumerical analysis010102 general mathematicsMathematical analysisRotational symmetryChemotaxiConcentricmedicine.disease01 natural sciencesQuantitative Biology::Cell Behavior010305 fluids & plasmasNonlinear systemAmplitudeAxisymmetric solution0103 physical sciencesmedicineMathematics (all)Multiple sclerosi0101 mathematicsEarly phaseBifurcationRicerche di Matematica
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Experimental and numerical study of noise effects in a FitzHugh–Nagumo system driven by a biharmonic signal

2013

Abstract Using a nonlinear circuit ruled by the FitzHugh–Nagumo equations, we experimentally investigate the combined effect of noise and a biharmonic driving of respective high and low frequency F and f. Without noise, we show that the response of the circuit to the low frequency can be maximized for a critical amplitude B∗ of the high frequency via the effect of Vibrational Resonance (V.R.). We report that under certain conditions on the biharmonic stimulus, white noise can induce V.R. The effects of colored noise on V.R. are also discussed by considering an Ornstein–Uhlenbeck process. All experimental results are confirmed by numerical analysis of the system response.

PhysicsArtificial neural networkGeneral MathematicsApplied MathematicsNumerical analysisAcousticsMathematical analysisGeneral Physics and AstronomyStatistical and Nonlinear PhysicsWhite noiseLow frequencyNonlinear systemAmplitudeColors of noiseBiharmonic equationChaos, Solitons & Fractals
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Numerical Relativistic Hydrodynamics

2008

High Resolution Shock Capturing (HRSC) techniques achieve highly accurate numerical approximations (formally second order or better) in smooth regions of the flow, and capture the motion of unresolved steep gradients without creating spurious oscillations. I will show how these techniques have been extended to relativistic hydrodynamics, making it possible to explore some challenging astrophysical scenarios. I will review recent literature concerning the main properties of different special relativistic Riemann solvers, and discuss several test problems which are commonly used to evaluate the performance of numerical methods in relativistic hydrodynamics. In the second part, I will illustra…

PhysicsBlack holeLorentz factorsymbols.namesakeClassical mechanicsRiemann problemActive galactic nucleusAccretion (meteorology)Flow (mathematics)Astrophysics::High Energy Astrophysical PhenomenaNumerical analysissymbolsRiemann solver
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Towards an understanding of discrete ambiguities in truncated partial wave analyses

2017

It is well known that the observables in a single-channel scattering problem remain invariant once the amplitude is multiplied by an overall energy- and angle-dependent phase. This invariance is called the continuum ambiguity and acts on the infinite partial wave set. It has also long been known that, in the case of a truncated partial wave set, another invariance exists, originating from the replacement of the roots of partial wave amplitudes with their complex conjugate values. This discrete ambiguity is also known as the Omelaenko-Gersten-type ambiguity. In this paper, we show that for scalar particles, discrete ambiguities are just a subset of continuum ambiguities with a specific phase…

PhysicsComplex conjugateContinuum (measurement)Nuclear Theory010308 nuclear & particles physicsScatteringNumerical analysismedia_common.quotation_subjectFOS: Physical sciencesObservableComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)AmbiguityInvariant (physics)01 natural sciencesNuclear Theory (nucl-th)partial wave decomposition continuum and discrete ambiguitiesTheoretical physicsAmplitude0103 physical sciences010306 general physicsmedia_common
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