Search results for "rotational symmetry"

showing 10 items of 58 documents

Multi-directional vs. mono-directional multi-step strategies for single point incremental forming of non-axisymmetric components

2020

Abstract Multi Stage approach is used in Single Point Incremental Forming (SPIF) to overcome one of the main forming limitations, namely the maximum wall angle, characterizing the single stage process. In this paper, different multi-path strategies for the production of parts with flat edges are considered in order to evaluate the best solution in terms of feasibility and geometrical accuracy of the final part: A) mono-directional incremental draw angle; B) mono-directional incremental draw angle with increasing part side; C) Multi-directional approach with non-horizontal path planes. Strain evaluation by means of CGA (Circular Grid Analysis) and defect analysis have been carried out in ord…

FEM0209 industrial biotechnologyMaterials scienceAluminium alloySingle stageStrategy and ManagementGrid analysisNumerical analysisIncremental formingRotational symmetryGeometry02 engineering and technologyManagement Science and Operations Research021001 nanoscience & nanotechnologyMulti-step toolpathIndustrial and Manufacturing EngineeringFinite element methodMulti stage020901 industrial engineering & automationMulti directionalSingle point0210 nano-technologyJournal of Manufacturing Processes
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Shape transitions of giant liposomes induced by an anisotropic spontaneous curvature

2000

International audience; We explore how a magnetic field breaks the symmetry of an initially spherical giant liposome filled with a magnetic colloid. The condition of rotational symmetry along the field axis leads either to a prolate or to an oblate ellipsoid. We demonstrate that an electrostatic interaction between the nanoparticles and the membrane triggers the shape transition. PACS numbers: 75.

Field (physics)Static ElectricityRotational symmetryFOS: Physical sciencesNanoparticle02 engineering and technologyCondensed Matter - Soft Condensed Matter[CHIM.INOR]Chemical Sciences/Inorganic chemistryCurvatureFerric Compounds01 natural sciencesMagneticsColloid0103 physical sciencesColloids010306 general physicsAnisotropyDebye lengthPhysicsCondensed matter physicsOsmolar Concentration[CHIM.MATE]Chemical Sciences/Material chemistryModels Theoretical021001 nanoscience & nanotechnologyGiant liposomesSymmetry (physics)Magnetic field[CHIM.POLY]Chemical Sciences/PolymersClassical mechanicsLiposomesMagnetic nanoparticlesPhosphatidylcholinesSoft Condensed Matter (cond-mat.soft)AnisotropySpontaneous curvature0210 nano-technology[PHYS.COND.CM-SCM]Physics [physics]/Condensed Matter [cond-mat]/Soft Condensed Matter [cond-mat.soft]Physical Review E
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Matched asymptotic solution for the solute boundary layer in a converging axisymmetric stagnation point flow

2007

Abstract A novel boundary-layer solution is obtained by the method of matched asymptotic expansions for the solute distribution at a solidification front represented by a disk of finite radius R 0 immersed in an axisymmetric converging stagnation point flow. The detailed analysis reveals a complex internal structure of the boundary layer consisting of eight subregions. The development of the boundary layer starts from the rim region where the concentration, according to the obtained similarity solution, varies with the radius r along the solidification front as ∼ln 1/3 ( R 0 / r ). At intermediate radii, where the corresponding concentration is found to vary as ∼ln( R 0 / r ), the boundary …

Fluid Flow and Transfer ProcessesConvectionMaterials scienceMechanical EngineeringRotational symmetryInner coreThermodynamicsGeometryRadiusCondensed Matter PhysicsSimilarity solutionMethod of matched asymptotic expansionsPhysics::Fluid DynamicsBoundary layerDiffusion (business)
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A mathematical simulation of high temperature induction heating of electroconductive solids

2007

The mathematical model of non-stationary coupled electromagnetic and thermal processes in polarizable and magnetizable axisymmetric electroconductive solids subjected to electromagnetic field generated by external currents is proposed. The processes parameters are connected through heat sources and temperature dependence of material characteristics. The problem is solved by finite element method. The process of induction heating of a finite steel cylinder is considered.

Fluid Flow and Transfer ProcessesElectromagnetic fieldInduction heatingMaterials scienceMathematical modelMechanical EngineeringRotational symmetryThermodynamicsMechanicsCondensed Matter PhysicsFinite element methodPolarizabilityThermalElectrical conductorInternational Journal of Heat and Mass Transfer
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Independent friction-restitution modeling of two-disk collisions

2021

[EN] The oblique collisions between two axisymmetric disks moving on a flat horizontal surface are described in terms of impact modeling based on the assumption that normal and tangential restitution mechanisms operate independently of friction. Describing these mechanisms in terms of the usual Coulomb formulation, the model allows for an interpretation of some ¿anomalous¿ experimental data reported in the literature. These experimental data, corresponding to the variation of the coefficients of friction and tangential restitution with the impact angle, remained unexplained in classic formulations, are understood within the framework of the independent friction-restitution closure. Experime…

Fluid Flow and Transfer ProcessesPhysicsSurface (mathematics)Mechanical EngineeringRolling resistanceComputational MechanicsRotational symmetryExperimental dataOblique caseMechanicsCondensed Matter PhysicsRestitutionClosure (computer programming)Mechanics of MaterialsPINTURACoulomb
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Numerically solving the relativistic Grad–Shafranov equation in Kerr spacetimes: numerical techniques

2018

The study of the electrodynamics of static, axisymmetric and force-free Kerr magnetospheres relies vastly on solutions of the so called relativistic Grad-Shafranov equation (GSE). Different numerical approaches to the solution of the GSE have been introduced in the literature, but none of them has been fully assessed from the numerical point of view in terms of efficiency and quality of the solutions found. We present a generalization of these algorithms and give detailed background on the algorithmic implementation. We assess the numerical stability of the implemented algorithms and quantify the convergence of the presented methodology for the most established setups (split-monopole, parab…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGeneralizationRotational symmetryFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyMagnetic fieldGrad–Shafranov equationQuality (physics)Space and Planetary Science0103 physical sciencesConvergence (routing)Applied mathematicsPoint (geometry)Astrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsNumerical stabilityMonthly Notices of the Royal Astronomical Society
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Simulations of an inhomogeneous stellar wind interacting with a pulsar wind in a binary system

2014

Binary systems containing a massive star and a non-accreting pulsar present strong interaction between the stellar and the pulsar winds. The properties of this interaction, which largely determine the non-thermal radiation in these systems, strongly depend on the structure of the stellar wind, which can be clumpy or strongly anisotropic, as in Be stars. We study numerically the influence of inhomogeneities in the stellar wind on the structure of the two-wind interaction region. We carried out for the first time axisymmetric, relativistic hydrodynamical simulations, with Lorentz factors of ~6 and accounting for the impact of instabilities, to study the impact in the two-wind interaction stru…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::High Energy Astrophysical PhenomenaLorentz transformationStrong interactionRotational symmetryFOS: Physical sciencesBinary numberAstronomy and AstrophysicsContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakePulsar13. Climate actionSpace and Planetary SciencePhysics::Space PhysicssymbolsAstrophysics::Solar and Stellar AstrophysicsDensity contrastAstrophysics - High Energy Astrophysical PhenomenaAnisotropyPhysics::Atmospheric and Oceanic PhysicsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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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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Numerical study of transient behaviour of molten zone during industrial FZ process for large silicon crystal growth

2004

The fully transient axisymmetric model has been developed for calculation of phase boundaries in large (up to 200 mm diameter) industrial floating zone (FZ) silicon single crystal growth with the needle-eye technique. The transient model is implemented in a specialized computer program. The model and program are based on a previously developed model and program for steady-state FZ process calculations. This transient approach allows studying of such substantially time-dependent process phases as the growth of the starting and ending cones of the crystal rod, which are particularly important for growth of large crystals in practice. Numerous calculations are carried out and the results for r…

Materials scienceSiliconComputer programProcess (computing)Rotational symmetrychemistry.chemical_elementMineralogyMechanicsCondensed Matter PhysicsInorganic ChemistryMonocrystalline siliconCrystalchemistryPhase (matter)Materials ChemistryTransient (oscillation)Journal of Crystal Growth
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Crystal shape 2D modeling for transient CZ silicon crystal growth

2013

Abstract A non-stationary axisymmetric model of Czochralski silicon single crystal growth is presented. The model describes transient behavior of crystal–melt, melt–gas and crystal–gas interfaces in connection with PID-based control of crystal diameter by changing crystal pulling velocity and heater power. To calculate significant crystal shape changes, unstructured finite element mesh is used in crystal and melt together with automatic element size control. Heater temperature changes are modeled with a simplified integral model. A numerical simulation example of start cone growth is given.

Materials scienceSiliconComputer simulationRotational symmetryPhysics::Opticschemistry.chemical_elementCrystal growthMechanicsCondensed Matter PhysicsFinite element methodPower (physics)Inorganic ChemistryCrystalCrystallographychemistryCondensed Matter::SuperconductivityMaterials ChemistryTransient (oscillation)Journal of Crystal Growth
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