Search results for " Hydrodynamic"

showing 10 items of 121 documents

Stability of hydrodynamical relativistic planar jets : II. Long-term nonlinear evolution

2004

In this paper we continue our study of the Kelvin-Helmholtz (KH) instability in relativistic planar jets following the long-term evolution of the numerical simulations which were introduced in Paper I. The models have been classified into four classes (I to IV) with regard to their evolution in the nonlinear phase, characterized by the process of jet/ambient mixing and momentum transfer. Models undergoing qualitatively different non-linear evolution are clearly grouped in well-separated regions in a jet Lorentz factor/jet-to-ambient enthalpy diagram. Jets with a low Lorentz factor and small enthalpy ratio are disrupted by a strong shock after saturation. Those with a large Lorentz factor an…

Lorentz transformationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsKinetic energyInstabilityMomentumsymbols.namesakeJetsMixing (physics)PhysicsJet (fluid)Momentum transferAstrophysics (astro-ph)Galaxies ; Jets ; Hydrodynamics ; InstabilitiesAstronomy and AstrophysicsMechanicsGalaxies:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Lorentz factorSpace and Planetary ScienceInstabilitiessymbolsHydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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A new general relativistic magnetohydrodynamics code for dynamical spacetimes

2008

We present a new numerical code which solves the general relativistic magneto-hydrodynamics (GRMHD) equations coupled to the Einstein equations for the evolution of a dynamical spacetime within the conformally-flat approximation. This code has been developed with the main objective of studying astrophysical scenarios in which both, high magnetic fields and strong gravitational fields appear, such as the magneto-rotational collapse of stellar cores, the collapsar model of GRBs, and the evolution of neutron stars. The code is based on an existing and thoroughly tested purely hydrodynamics code and on its extension to accommodate weakly magnetized fluids (passive magnetic field approximation).…

Magnetohydrodynamics (MHD)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesConformal mapAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyRelativityGravitational fieldUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GravitaciónPhysicsnumerical [Methods]SpacetimeSolenoidal vector fieldGravitation; Hydrodynamics; Magnetohydrodynamics (MHD); Methods : numerical; Relativity; Stars : supernovae : generalsupernovae : general [Stars]Astrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Gravitación [UNESCO]Magnetic fieldNeutron starClassical mechanicsSpace and Planetary ScienceHydrodynamicsCircular symmetryMagnetohydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasGravitation:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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General relativistic simulations of pasive-magneto-rotational core collapse with microphysics

2007

This paper presents results from axisymmetric simulations of magneto-rotational stellar core collapse to neutron stars in general relativity using the passive field approximation for the magnetic field. These simulations are performed using a new general relativistic numerical code specifically designed to study this astrophysical scenario. The code is based on the conformally-flat approximation of Einstein's field equations and conservative formulations of the magneto-hydrodynamics equations. The code has been recently upgraded to incorporate a tabulated, microphysical equation of state and an approximate deleptonization scheme. This allows us to perform the most realistic simulations of m…

Magnetohydrodynamics (MHD)General relativityRotational symmetryFOS: Physical sciencesGravitation ; Hydrodynamics ; Magnetohydrodynamics (MHD) ; Numerical ; Stars ; Supernovae ; RelativityAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)UNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsInstabilityGeneral Relativity and Quantum CosmologyRelativityStellar evolutionPhysicsNumericalMicrophysicsAstrophysics (astro-ph)Astronomy and AstrophysicsStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Magnetic fieldComputational physicsNeutron starSupernovaeSpace and Planetary ScienceHydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]DynamoGravitation
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A Meshless Approach for Electromagnetic Simulation of Metallic Carbon Nanotubes

2009

In this paper, a study on the electromagnetic behaviour of a single wall carbon nanotube model is described. The electrons available for conduction are treated as a thin cylindrical layer fluid and their motion is described by means of classical hydrodynamics equations in linearized form. These equations are solved in time domain using the Smoothed Particle Hydrodynamics method. The method suitably handled runs on GRID environment.

Materials scienceElectromagneticsApplied MathematicsElectromagnetic Simulationchemistry.chemical_elementMetallic Carbon NanotubeGeneral ChemistryMechanicsCarbon nanotubeElectronThermal conductionMeshlelaw.inventionSmoothed-particle hydrodynamicsSettore MAT/08 - Analisi NumericaSettore ING-IND/31 - ElettrotecnicaClassical mechanicschemistrylawMeshfree methodsTime domainCarbon
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On the use of a meshless solver for PDEs governing electromagnetic transients

2009

In this paper some key elements of the Smoothed Particle Hydrodynamics methodology suitably reformulated for analyzing electromagnetic transients are investigated. The attention is focused on the interpolating smoothing kernel function which strongly influences the computational results. Some issues are provided by adopting the polynomial reproducing conditions. Validation tests involving Gaussian and cubic B-spline smoothing kernel functions in one and two dimensions are reported.

Mathematical optimizationPolynomialPartial differential equationApplied MathematicsB-splineNumerical analysisGaussianMeshless particle methodSmoothed Particle Hydrodynamics methodMaxwell's equationSolverSmoothed-particle hydrodynamicsSettore MAT/08 - Analisi NumericaSettore ING-IND/31 - ElettrotecnicaComputational Mathematicssymbols.namesakeElectromagnetic transientsymbolsApplied mathematicsSmoothingMathematicsApplied Mathematics and Computation
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Fluid-structure interaction approach with smoothed particle hydrodynamics and particle-spring systems

2022

This paper presents a novel three-dimensional fluid-structure interaction (FSI) approach, where the meshless smoothed particle hydrodynamics (SPH) method is used to simulate the motion of incompressible fluid flows, whilst structures are represented by a simplified approach based on particle-spring systems. The proposed FSI technique allows to use independent spatial-temporal resolutions for the fluid and structural computational domains. The particle-spring elastic constants are calibrated and relationships with the mechanical material properties, Young's modulus and Poisson's ratio, are determined. Fluid and structure computational domains are separated by interfaces made of triangular el…

Mechanics of MaterialsMechanical EngineeringComputational MechanicsGeneral Physics and AstronomySmoothed particle hydrodynamics (SPH) Fluid-structure interaction (FSI) Particle-spring systems Particle-based FSI FSI benchmarkComputer Science ApplicationsSettore ICAR/01 - Idraulica
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Ba/Ca evolution in water masses of the Mediterranean late Neogene

2008

A Mediterranean composite sedimentary record was analyzed for Ba/Ca ratios on carbonate shells of Orbulina universa planktonic foraminifer (Ba/Ca) carb providing the opportunity to study and assess the extent of freshwater inputs on the basin and possible impacts on its dynamics during the Tortonian to Recent period. A number of scanning electron microscope analyses and auxiliary trace element measurements (Mn, Sr, and Mg), obtained from the same samples, exclude important diagenetic effects on the studied biogenic carbonates and corroborate the reliability of (Ba/Ca) carb ratios in foraminifera calcite as indicators of seawater source components during the studied interval. A long-term tre…

Mediterranean sealate Neogene(Ba/Ca)carb ratiosalinity change3-D hydrodynamics
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A derivation of the isothermal quantum hydrodynamic equations using entropy minimization

2005

Isothermal quantum hydrodynamic equations of order O(h 2 ) using the quantum entropy minimization method recently developed by Degond and Ringhofer are derived. The equations have the form of the usual quantum hydrodynamic model including a correction term of order O(h 2 ) which involves the vorticity. If the initial vorticity is of order 0(h), the standard model is obtained up to order O(h 4 ). The derivation is based on a careful expansion of the quantum equilibrium obtained from the entropy minimization in powers of h 2 .

Minimisation (psychology)Standard Model (mathematical formulation)Classical mechanicsQuantum hydrodynamicsApplied MathematicsComputational MechanicsOrder (ring theory)Von Neumann entropyVorticityQuantumIsothermal processMathematical physicsMathematicsZAMM
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Validation of models for sprays

2016

We consider complex fluids consisting of a dispersed phase (solid particles or liquid droplets) immersed in a gas. A class of models describing the dynamics of such a kind of systems is given by a system of partial differential equations where a kinetic equation, describing the dispersed phase, is coupled to a fluid equation for the background gas. The coupling is given by the drag force exerted by the gas on the dispersed phase. Within this class, we shall analyse the case where the kinetic equation is a Vlasov-type equation and the fluid equation are of Stokes or Navier-Stokes type. We shall discuss the validation problem for this class of models, i.e. the derivation of the equations of t…

Modelling spray validation of hydrodynamical modelsSettore MAT/07 - Fisica Matematica
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A Smoothed Particle Image Reconstruction method

2010

Many image processing techniques work with scattered data distribution usually employing grid based methods leading to numerical problems. To address this issue, a numerical method avoiding mesh generation can be used. Such a method performs an integral representation by means of a smoothing kernel function and, in the discrete formulation, involves domain particles. In this paper the meshless Smoothed Particle Hydrodynamics method is proposed in the Image Reconstruction context and a new computational strategy called Smoothed Particle Image Reconstruction is presented; the new method is based on a scatter approach and several innovative ideas are introduced in order to improve the computat…

Nearest neighboring searchMathematical optimizationAlgebra and Number TheoryConsistency restoringNumerical analysisMeshless particle methodContext (language use)Image processingFunction (mathematics)Iterative reconstructionSmoothed-particle hydrodynamicsSettore MAT/08 - Analisi NumericaComputational MathematicsImage processingMesh generationImage reconstruction reconstructionTheory of computationSmoothed particle Hydrodinamics methodAlgorithmMathematicsCalcolo
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