Search results for "physics.flu-dyn"

showing 10 items of 64 documents

Surface sulci in squeezed soft solids

2013

The squeezing of soft solids, the constrained growth of biological tissues, and the swelling of soft elastic solids such as gels can generate large compressive stresses at their surfaces. This causes the otherwise smooth surface of such a solid to become unstable when its stress exceeds a critical value. Previous analyses of the surface instability have assumed two-dimensional plane-strain conditions, but in experiments isotropic stresses often lead to complex three-dimensional sulcification patterns. Here we show how such diverse morphologies arise by numerically modeling the lateral compression of a rigidly clamped elastic layer. For incompressible solids, close to the instability thresho…

Surface (mathematics)Materials sciencemekaniikkata114Condensed matter physicsbusiness.industryPhysicsIsotropyFluid Dynamics (physics.flu-dyn)General Physics and AstronomyFOS: Physical sciencesPhysics - Fluid DynamicsCondensed Matter - Soft Condensed MatterCritical valueMechanicsInstabilityStress (mechanics)OpticsBucklingPhase (matter)CompressibilitySoft Condensed Matter (cond-mat.soft)fysiikkabusiness
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Dynamic mode decomposition of magnetohydrodynamic bubble chain flow in a rectangular vessel

2021

We demonstrate the first application of dynamic mode decomposition (DMD) to bubble flow with resolved dynamic liquid/gas boundaries. Specifically, we have applied DMD to the output of numerical simulations for a system where chains of bubbles ascend through a rectangular liquid metal vessel. Flow patterns have been investigated in the vessel and bubble reference frames. We show how gas flow rate and applied magnetic affect bubble wake flow and larger-scale flow structures within the liquid metal vessel by examining the velocity field mode statistics over trajectory time and total flow time as well as the computed mode velocity fields. The results of this proof-of-concept study indicate that…

Fluid Flow and Transfer ProcessesPhysicsLiquid metalMechanical EngineeringBubbleComputational MechanicsFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesMechanicsPhysics - Fluid DynamicsWakeCondensed Matter PhysicsVolumetric flow ratePhysics::Fluid DynamicsFlow (mathematics)Mechanics of MaterialsDynamic mode decompositionVector fieldMagnetohydrodynamic drive
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Multicomponent relativistic dissipative fluid dynamics from the Boltzmann equation

2022

We derive multicomponent relativistic second-order dissipative fluid dynamics from the Boltzmann equations for a reactive mixture of $N_{\text{spec}}$ particle species with $N_q$ intrinsic quantum numbers (e.g. electric charge, baryon number, and strangeness) using the method of moments. We obtain the continuity equations for multiple conserved charges as well as the conservation equations for the total energy and momentum in the single-fluid approximation. These $4+N_q$ conservation laws are closed by deriving the second-order equations of motion for the dissipative quantities in the $(10+4N_q)$-moment approximation. The resulting fluid-dynamical equations are formally similar to those of …

Nuclear Theory (nucl-th)mallintaminenHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear TheoryFluid Dynamics (physics.flu-dyn)fluiditFOS: Physical sciencesPhysics - Fluid Dynamicshiukkasfysiikkavahva vuorovaikutus
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History and results of the Riga dynamo experiments

2008

On 11 November 1999, a self-exciting magnetic eigenfield was detected for the first time in the Riga liquid sodium dynamo experiment. We report on the long history leading to this event, and on the subsequent experimental campaigns which provided a wealth of data on the kinematic and the saturated regime of this dynamo. The present state of the theoretical understanding of both regimes is delineated, and some comparisons with other laboratory dynamo experiments are made.

Astrophysics (astro-ph)Fluid Dynamics (physics.flu-dyn)General EngineeringFOS: Physical sciencesEnergy Engineering and Power TechnologyChamp magnetiqueGeophysicsPhysics - Fluid DynamicsAstrophysicsPhysics::GeophysicsPhysics::Fluid DynamicsNuclear magnetic resonanceDynamo theoryMagnetohydrodynamicsGeologyDynamo
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The Mach cone signal and energy deposition scenarios in linearized hydrodynamics

2010

Particle correlation measurements associated with a hard or semi-hard trigger in heavy-ion collisions may reflect Mach cone shockwaves excited in the bulk medium by partonic energy loss. This is of great interest because, when compared with theory, such measurements can provide information on the transport properties of the medium. Specifically, the formation of Mach cone shockwaves is sensitive to the viscosity and speed of sound, as well as the detailed nature of the jet medium interaction. However, modeling the physics of shockwave excitation to obtain a meaningful comparison with the measured correlations is very challenging since the correlations arise from an interplay of perturbative…

Shock wavePhysicsNuclear and High Energy PhysicsNuclear TheoryFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesFluid mechanicsPartonPhysics - Fluid DynamicsComputational physicsMomentumPhysics::Fluid DynamicsNuclear Theory (nucl-th)High Energy Physics - Phenomenologysymbols.namesakeClassical mechanicsHigh Energy Physics - Phenomenology (hep-ph)Mach numberExcited stateSpeed of soundQuark–gluon plasmasymbols
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Cross-stream migration of a Brownian droplet in a polymer solution under Poiseuille flow

2018

The migration of a Brownian fluid droplet in a parallel-plate microchannel was investigated using dissipative particle dynamics computer simulations. In a Newtonian solvent, the droplet migrated toward the channel walls due to inertial effects at the studied flow conditions, in agreement with theoretical predictions and recent simulations. However, the droplet focused onto the channel centerline when polymer chains were added to the solvent. Focusing was typically enhanced for longer polymers and higher polymer concentrations with a nontrivial flow-rate dependence due to droplet and polymer deformability. Brownian motion caused the droplet position to fluctuate with a distribution that prim…

Materials scienceFOS: Physical sciences02 engineering and technologyCondensed Matter - Soft Condensed Matter010402 general chemistry01 natural sciencesPhysics::Fluid DynamicsNewtonian fluidPhysics::Atomic and Molecular ClustersBrownian motionchemistry.chemical_classificationMicrochannelDissipative particle dynamicsFluid Dynamics (physics.flu-dyn)General ChemistryPolymerMechanicsPhysics - Fluid Dynamics021001 nanoscience & nanotechnologyCondensed Matter PhysicsHagen–Poiseuille equation0104 chemical sciencesShear rateLift (force)Condensed Matter::Soft Condensed MatterchemistrySoft Condensed Matter (cond-mat.soft)0210 nano-technology
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

2018

We propose a novel method to constrain turbulence and bulk motions in massive galaxies, groups and clusters, exploring both simulations and observations. As emerged in the recent picture of the top-down multiphase condensation, the hot gaseous halos are tightly linked to all other phases in terms of cospatiality and thermodynamics. While hot halos (10^7 K) are perturbed by subsonic turbulence, warm (10^4 K) ionized and neutral filaments condense out of the turbulent eddies. The peaks condense into cold molecular clouds (< 100 K) raining in the core via chaotic cold accretion (CCA). We show all phases are tightly linked via the ensemble (wide-aperture) velocity dispersion along the line o…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics01 natural sciencesSpectral lineGalaxy groupAbsorption (logic)010303 astronomy & astrophysicsLine (formation)hydrodynamicPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Velocity dispersionPhysics - Fluid DynamicsComputational Physics (physics.comp-ph)active [galaxies]astro-ph.COspectroscopic [techniques]Astrophysics - High Energy Astrophysical PhenomenaPhysics - Computational PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics[ INFO ] Computer Science [cs]Cosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAgalaxies: activeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsISM [radio lines]0103 physical sciences[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]/dk/atira/pure/subjectarea/asjc/1900/1912[INFO]Computer Science [cs]Astrophysics::Galaxy Astrophysicsradio lines: ISM010308 nuclear & particles physicsMolecular cloudturbulenceFluid Dynamics (physics.flu-dyn)Astronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesX-rays: galaxies: clusterGalaxyAccretion (astrophysics)[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]physics.flu-dynphysics.comp-phSpace and Planetary ScienceX-rays: galaxies: clustersAstrophysics of Galaxies (astro-ph.GA)hydrodynamics/dk/atira/pure/subjectarea/asjc/3100/3103galaxies: clusters [X-rays][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]techniques: spectroscopic
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Resolving gas bubbles ascending in liquid metal from low-SNR neutron radiography images

2021

We demonstrate a new image processing methodology for resolving gas bubbles travelling through liquid metal from dynamic neutron radiography images with an intrinsically low signal-to-noise ratio. Image pre-processing, denoising and bubble segmentation are described in detail, with practical recommendations. Experimental validation is presented—stationary and moving reference bodies with neutron-transparent cavities are radiographed with imaging conditions representative of the cases with bubbles in liquid metal. The new methods are applied to our experimental data from previous and recent imaging campaigns, and the performance of the methods proposed in this paper is compared against our p…

FOS: Computer and information sciencesLiquid metalTechnologyMaterials scienceQH301-705.5low signal-to-noise ratio (SNR)BubbleAcousticsNoise reductionQC1-999Computer Vision and Pattern Recognition (cs.CV)dynamic neutron imagingComputer Science - Computer Vision and Pattern Recognitionmetohydrodynamics (MHD)FOS: Physical sciencesImage processingdenoisingGeneral Materials ScienceSegmentationBiology (General)InstrumentationQD1-999Fluid Flow and Transfer ProcessesProcess Chemistry and TechnologyNeutron imagingTPhysicssegmentationGeneral EngineeringFluid Dynamics (physics.flu-dyn)Experimental dataPhysics - Fluid DynamicsEngineering (General). Civil engineering (General)Computer Science Applicationsimage processingtwo-phase flowChemistryliquid metalComputer Science::Computer Vision and Pattern RecognitionTwo-phase flowTA1-2040bubble flow
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Magnetohydrodynamic experiments on cosmic magnetic fields

2008

It is widely known that cosmic magnetic fields, i.e. the fields of planets, stars, and galaxies, are produced by the hydromagnetic dynamo effect in moving electrically conducting fluids. It is less well known that cosmic magnetic fields play also an active role in cosmic structure formation by enabling outward transport of angular momentum in accretion disks via the magnetorotational instability (MRI). Considerable theoretical and computational progress has been made in understanding both processes. In addition to this, the last ten years have seen tremendous efforts in studying both effects in liquid metal experiments. In 1999, magnetic field self-excitation was observed in the large scale…

PhysicsStructure formationApplied MathematicsAstrophysics (astro-ph)Fluid Dynamics (physics.flu-dyn)Computational MechanicsFOS: Physical sciencesPhysics - Fluid DynamicsAstrophysicsInstabilityComputational physicsMagnetic fieldPhysics::Fluid DynamicsMagnetorotational instabilityDynamo theoryMagnetohydrodynamicsCouette flowDynamo
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On the variations of acoustic absorption peak with particle velocity in micro-perforated panels at high level of excitation.

2010

The acoustic behavior of micro-perforated panels (MPP) is studied theoretically and experimentally at high level of pressure excitation. A model based on Forcheimer's regime of flow velocity in the perforations is proposed. This model is valid at relatively high Reynolds numbers and low Mach numbers. The experimental method consists in measuring the acoustical pressure at three different positions in an impedance tube, the two measurement positions usually considered in an impedance tube and one measurement in the vicinity of the rear surface of the MPP. The impedance tube is equipped with a pressure driver instead of the usual loudspeaker and capable of delivering a high sound pressure lev…

Absorption (acoustics)Materials scienceAcoustics and UltrasonicsAcoustics[ PHYS.COND.CM-MS ] Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]FOS: Physical sciencesPhysics - Classical PhysicsPolypropylenes01 natural sciences010305 fluids & plasmasAbsorption[SPI]Engineering Sciences [physics]symbols.namesakeMotionArts and Humanities (miscellaneous)0103 physical sciencesPressureParticle velocitySound pressure010301 acoustics[ PHYS.MECA.ACOU ] Physics [physics]/Mechanics [physics]/Acoustics [physics.class-ph][SPI.ACOU]Engineering Sciences [physics]/Acoustics [physics.class-ph][ SPI.ACOU ] Engineering Sciences [physics]/Acoustics [physics.class-ph]Construction MaterialsAirFluid Dynamics (physics.flu-dyn)Classical Physics (physics.class-ph)Reynolds numberPhysics - Fluid DynamicsAcousticsModels TheoreticalSound intensity[PHYS.MECA.ACOU]Physics [physics]/Mechanics [physics]/Acoustics [physics.class-ph]Mach numberFlow velocityNonlinear DynamicsSteelFacility Design and Construction[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]symbolsLinear ModelsAcoustic impedanceNoisePorosityThe Journal of the Acoustical Society of America
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