Search results for "Hydrodynamics"

showing 10 items of 390 documents

Flow properties and hydrodynamic interactions of rigid spherical microswimmers.

2017

We analyze a minimal model for a rigid spherical microswimmer and explore the consequences of its extended surface on the interplay between its self-propulsion and flow properties. The model is the first order representation of microswimmers, such as bacteria and algae, with rigid bodies and flexible propelling appendages. The flow field of such a microswimmer at finite distances significantly differs from that of a point-force (Stokeslet) dipole. For a suspension of microswimmers, we derive the grand mobility matrix that connects the motion of an individual swimmer to the active and passive forces and torques acting on all the swimmers. Our investigation of the mobility tensors reveals tha…

Collective behaviorStokesian dynamicsMovementFOS: Physical sciencesCondensed Matter - Soft Condensed MatterBacterial Physiological Phenomena01 natural sciencesQuantitative Biology::OtherModels Biological010305 fluids & plasmasQuantitative Biology::Cell Behavior0103 physical sciencesComputer SimulationPhysics - Biological Physics010306 general physicsSuspension (vehicle)Plant Physiological PhenomenaPhysicsPhysics::Biological PhysicsFluid Dynamics (physics.flu-dyn)EukaryotaPhysics - Fluid DynamicsFirst orderFlow fieldDipoleClassical mechanicsBiological Physics (physics.bio-ph)HydrodynamicsSoft Condensed Matter (cond-mat.soft)Flow propertiesPhysical review. E
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Magnetic fields in heavy ion collisions: flow and charge transport

2020

At the earliest times after a heavy-ion collision, the magnetic field created by the spectator nucleons will generate an extremely strong, albeit rapidly decreasing in time, magnetic field. The impact of this magnetic field may have detectable consequences, and is believed to drive anomalous transport effects like the Chiral Magnetic Effect (CME). We detail an exploratory study on the effects of a dynamical magnetic field on the hydrodynamic medium created in the collisions of two ultrarelativistic heavy-ions, using the framework of numerical ideal MagnetoHydroDynamics (MHD) with the ECHO-QGP code. In this study, we consider a magnetic field captured in a conducting medium, where the conduc…

Computer Science::Machine LearningParticle physicsPhysics and Astronomy (miscellaneous)Nuclear Theoryheavy ion collisionsFOS: Physical scienceslcsh:Astrophysicsmagnetic fieldshiukkasfysiikkamagneettikentätComputer Science::Digital Libraries01 natural sciencesElectric charge530Nuclear Theory (nucl-th)Statistics::Machine LearningHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466ddc:530lcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentEngineering (miscellaneous)Nuclear ExperimentPhysicsCharge conservation010308 nuclear & particles physicsElliptic flowCharge (physics)FermionMagnetic fieldDipoleHigh Energy Physics - PhenomenologyQuantum electrodynamicsComputer Science::Mathematical Softwarelcsh:QC770-798MagnetohydrodynamicsThe European Physical Journal C
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Highlighting numerical insights of an efficient SPH method

2018

Abstract In this paper we focus on two sources of enhancement in accuracy and computational demanding in approximating a function and its derivatives by means of the Smoothed Particle Hydrodynamics method. The approximating power of the standard method is perceived to be poor and improvements can be gained making use of the Taylor series expansion of the kernel approximation of the function and its derivatives. The modified formulation is appealing providing more accurate results of the function and its derivatives simultaneously without changing the kernel function adopted in the computation. The request for greater accuracy needs kernel function derivatives with order up to the desidered …

Computer scienceApplied MathematicsGaussianComputation010103 numerical & computational mathematicsFunction (mathematics)01 natural sciences010101 applied mathematicsSmoothed-particle hydrodynamicsComputational Mathematicssymbols.namesakeSettore MAT/08 - Analisi NumericaKernel based methods Smoothed Particle Hydrodynamics Accuracy Convergence Improved fast Gaussian transform.Convergence (routing)symbolsTaylor seriesGaussian function0101 mathematicsFocus (optics)Algorithm
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A multi-domain approach for smoothed particle hydrodynamics simulations of highly complex flows

2018

Abstract An efficient and accurate method is proposed to solve the incompressible flow momentum and continuity equations in computational domains partitioned into subdomains in the framework of the smoothed particle hydrodynamics method. The procedure does not require any overlap of the subdomains, which would result in the increase of the computational effort. Perfectly matching solutions are obtained at the surfaces separating neighboring blocks. The block interfaces can be both planar and curved surfaces allowing to easily decompose even geometrically complex domains. The smoothing length of the kernel function is maintained constant in each subdomain, while changing between blocks where…

Computer scienceComputational MechanicsGeneral Physics and AstronomyBoundary condition010103 numerical & computational mathematics01 natural sciencesSettore ICAR/01 - IdraulicaMomentumSmoothed-particle hydrodynamicsPhysics and Astronomy (all)Smoothed particle hydrodynamicIncompressible flowComputational mechanicsMechanics of MaterialDomain decomposition0101 mathematicsMirror particleComputational MechanicConservation of massISPHBlock (data storage)Mechanical EngineeringComputer Science Applications1707 Computer Vision and Pattern RecognitionDomain decomposition methodsComputer Science Applications010101 applied mathematicsMechanics of MaterialsMulti-blockAlgorithmSmoothingComputer Methods in Applied Mechanics and Engineering
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Towards an Efficient Implementation of an Accurate SPH Method

2020

A modified version of the Smoothed Particle Hydrodynamics (SPH) method is considered in order to overcome the loss of accuracy of the standard formulation. The summation of Gaussian kernel functions is employed, using the Improved Fast Gauss Transform (IFGT) to reduce the computational cost, while tuning the desired accuracy in the SPH method. This technique, coupled with an algorithmic design for exploiting the performance of Graphics Processing Units (GPUs), makes the method promising, as shown by numerical experiments.

Computer scienceGauss transformOrder (ring theory)Smoothed Particle Hydrodynamics Improved Fast Gauss Transform Graphics Processing UnitsSmoothed-particle hydrodynamicsSmoothed Particle Hydrodynamicssymbols.namesakeImproved Fast Gauss TransformGaussian functionsymbolsAlgorithm designGraphics Processing UnitsGraphicsAlgorithmComputingMethodologies_COMPUTERGRAPHICS
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Mesoscopic Simulations of Polyelectrolyte Electrophoresis in Nanochannels

2011

We present the results of mesoscopic dissipative particle dynamics (DPD) simulations of coupled electrohydrodynamic phenomena on the micro- and nanoscale. The effects of electroosmotic flow and slippage combined with polyelectrolyte electrophoresis are investigated in detail, taking full account of hydrodynamic and electrostatic interactions. Our numerical results are in excellent agreement with analytical calculations.

Condensed Matter::Soft Condensed MatterMesoscopic physicsElectrophoresisChemical physicsComputer scienceDissipative particle dynamicsElectrohydrodynamicsElectrostaticsNanoscopic scalePolyelectrolyte
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Magnetic field emergence in mesogranular-sized exploding granules observed with SUNRISE/IMaX data

2011

We report on magnetic field emergences covering significant areas of exploding granules. The balloon-borne mission SUNRISE provided high spatial and temporal resolution images of the solar photosphere. Continuum images, longitudinal and transverse magnetic field maps and Dopplergrams obtained by IMaX onboard SUNRISE are analyzed by Local Correlation Traking (LCT), divergence calculation and time slices, Stokes inversions and numerical simulations are also employed. We characterize two mesogranular-scale exploding granules where $\sim$ 10$^{18}$ Mx of magnetic flux emerges. The emergence of weak unipolar longitudinal fields ($\sim$100 G) start with a single visible magnetic polarity, occupyi…

ConvectionPhysicsAdvectionFOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceTemporal resolutionSunriseAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsSolar and Stellar Astrophysics (astro-ph.SR)
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Magnetic field amplification and magnetically supported explosions of collapsing, non-rotating stellar cores

2014

We study the amplification of magnetic fields in the collapse and the post-bounce evolution of the core of a non-rotating star of 15 solar masses in axisymmetry. To this end, we solve the coupled equations of magnetohydrodynamics and neutrino transport in the two-moment approximation. The pre-collapse magnetic field is strongly amplified by compression in the infall. Initial fields of the order of 1010 G translate into proto-neutron star fields similar to the ones observed in pulsars, while stronger initial fields yield magnetar-like final field strengths. After core bounce, the field is advected through the hydrodynamically unstable neutrino-heating layer, where non-radial flows due to con…

ConvectionPhysicsMagnetic energyAdvectionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsMechanicsAstrophysicsAmplification factorInstabilityMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetohydrodynamicsSolar and Stellar Astrophysics (astro-ph.SR)Equipartition theoremMonthly Notices of the Royal Astronomical Society
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Mixed MHD convection and Tritium transport in fusion-relevant configurations

2005

Mixed MHD flow and Tritium transport were computed for a slender poloidal duct, representative of a DEMO HCLL blanket element. 2-D flow and temperature fields were computed in the duct's cross section under the assumption of parallel, fully developed flow, while Tritium concentration C was found by solving a fully 3-D problem with simplifying assumptions at the duct's ends. The spatial distribution of C depended on the intensity and direction of the forced flow. Significant peak factors were obtained if the net flow rate was so low that re-circulation occurred; C maxima were attained near the walls for upward flow, in the core region for downward flow.

ConvectionPhysicsMechanical EngineeringHCLL blanketMechanicsBlanketFusion powerMagnetohydrodynamicVolumetric flow ratePhysics::Fluid DynamicsNuclear physicsNuclear Energy and EngineeringCombined forced and natural convectionFlow conditioningGeneral Materials ScienceDuct (flow)Mixed convectionMagnetohydrodynamicsSettore ING-IND/19 - Impianti NucleariCivil and Structural Engineering
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Free-surface flows solved by means of SPH schemes with numerical diffusive terms

2010

A novel system of equations has been defined which contains diffusive terms in both the continuity and energy equations and, at the leading order, coincides with a standard weakly-compressible SPH scheme with artificial viscosity. A proper state equation is used to associate the internal energy variation to the pressure field and to increase the speed of sound when strong deformations/compressions of the fluid occur. The increase of the sound speed is associated to the shortening of the time integration step and, therefore, allows a larger accuracy during both breaking and impact events. Moreover, the diffusive terms allows reducing the high frequency numerical acoustic noise and smoothing …

Convergence testsGeneral Physics and AstronomyFluid-structure impact problemsSPH pressure evaluationSmoothed particle hydrodynamicsSystem of linear equations01 natural sciences010305 fluids & plasmasSmoothed-particle hydrodynamicsViscositySmoothed particle hydrodynamicSpeed of sound0103 physical sciencesConvergence testsFree-surface flow0101 mathematicsFree-surface flowsPhysicsInternal energyMechanics010101 applied mathematicsFluid-structure impact problemHardware and ArchitectureFree surfaceWeak-compressibilitySmoothing
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