Search results for "physics.flu-dyn"

showing 10 items of 64 documents

Influence of electromagnetic boundary conditions onto the onset of dynamo action in laboratory experiments

2009

We study the onset of dynamo action of the Riga and Karlsruhe experiments with the addition of an external wall, the electro-magnetic properties of which being different from those of the fluid in motion. We consider a wall of different thickness, conductivity and permeability. We also consider the case of a ferro-fluid in motion.

PhysicsFerrofluid[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Mechanics of the fluids [physics.class-ph][SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Fluid Dynamics (physics.flu-dyn)FOS: Physical sciences[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Physics - Fluid DynamicsConductivity01 natural sciences010305 fluids & plasmas[SPI.MECA.MEFL]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph]Physics::GeophysicsGeophysics (physics.geo-ph)Physics - GeophysicsPhysics::Fluid DynamicsClassical mechanicsPermeability (electromagnetism)0103 physical sciencesBoundary value problem[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph]010306 general physicsDynamo
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A physically based connection between fractional calculus and fractal geometry

2014

We show a relation between fractional calculus and fractals, based only on physical and geometrical considerations. The link has been found in the physical origins of the power-laws, ruling the evolution of many natural phenomena, whose long memory and hereditary properties are mathematically modelled by differential operators of non integer order. Dealing with the relevant example of a viscous fluid seeping through a fractal shaped porous medium, we show that, once a physical phenomenon or process takes place on an underlying fractal geometry, then a power-law naturally comes up in ruling its evolution, whose order is related to the anomalous dimension of such geometry, as well as to the m…

PhysicsFractal geometry; Fractional calculus; Fractional differential equation; Transport process; Physics and Astronomy (all)Transport proceFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesGeneral Physics and AstronomyPhysics - Fluid DynamicsFractional calculuDifferential operatorFractional differential equationAction (physics)Connection (mathematics)Fractional calculusFractal geometryPhysics and Astronomy (all)Nonlinear systemsymbols.namesakeSuperposition principleClassical mechanicsFractalBoltzmann constantsymbolsAnnals of Physics
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Anomalous dynamics triggered by a non-convex equation of state in relativistic flows

2017

The non-monotonicity of the local speed of sound in dense matter at baryon number densities much higher than the nuclear saturation density ($n_0 \approx 0.16\,$fm$^{-3}$) suggests the possible existence of a non-convex thermodynamics which will lead to a non-convex dynamics. Here, we explore the rich and complex dynamics that an equation of state (EoS) with non-convex regions in the pressure-density plane may develop as a result of genuinely relativistic effects, without a classical counterpart. To this end, we have introduced a phenomenological EoS, whose parameters can be restricted heeding to causality and thermodynamic stability constraints. This EoS shall be regarded as a toy-model wi…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsEquation of state (cosmology)Plane (geometry)Nuclear TheoryFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesAstronomy and AstrophysicsPhysics - Fluid DynamicsApprox01 natural sciencesCausality (physics)Complex dynamicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSpeed of sound0103 physical sciencesBaryon numberAstrophysics - High Energy Astrophysical PhenomenaRelativistic quantum chemistry010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Mathematical physics
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Relative importance of second-order terms in relativistic dissipative fluid dynamics

2013

In Denicol et al., Phys. Rev. D 85, 114047 (2012), the equations of motion of relativistic dissipative fluid dynamics were derived from the relativistic Boltzmann equation. These equations contain a multitude of terms of second order in Knudsen number, in inverse Reynolds number, or their product. Terms of second order in Knudsen number give rise to non-hyperbolic (and thus acausal) behavior and must be neglected in (numerical) solutions of relativistic dissipative fluid dynamics. The coefficients of the terms which are of the order of the product of Knudsen and inverse Reynolds numbers have been explicitly computed in the above reference, in the limit of a massless Boltzmann gas. Terms of …

PhysicsNuclear and High Energy PhysicsNuclear Theoryta114Lattice Boltzmann methodsFluid Dynamics (physics.flu-dyn)Reynolds numberFOS: Physical sciencesPhysics - Fluid DynamicsNonlinear Sciences::Cellular Automata and Lattice GasesBoltzmann equationPhysics::Fluid DynamicsNuclear Theory (nucl-th)High Energy Physics - Phenomenologysymbols.namesakeClassical mechanicsHigh Energy Physics - Phenomenology (hep-ph)Boltzmann constantsymbolsDissipative systemFluid dynamicsKnudsen numberDirect simulation Monte CarloPhysical Review D
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Magnetic micro-droplet in rotating field: numerical simulation and comparison with experiment

2017

Magnetic droplets obtained by induced phase separation in a magnetic colloid show a large variety of shapes when exposed to an external field. However, the description of shapes is often limited. Here we formulate an algorithm based on three dimensional boundary-integral equations for strongly magnetic droplets in a high-frequency rotating magnetic field, allowing us to find their figures of equilibrium in three dimensions. The algorithm is justified by a series of comparisons with known analytical results. We compare the calculated equilibrium shapes with experimental observations and find a good agreement. The main features of these observations are the oblate-prolate transition, the flat…

PhysicsRotating magnetic fieldComputer simulationField (physics)Mechanical EngineeringFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesMechanicsPhysics - Fluid DynamicsCondensed Matter - Soft Condensed MatterCondensed Matter Physics01 natural sciencesFlattening010305 fluids & plasmasMagnetic fieldSurface tensionViscosityDipoleMechanics of Materials0103 physical sciencesSoft Condensed Matter (cond-mat.soft)010306 general physics
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The exact solution of the Riemann problem with non-zero tangential velocities in relativistic hydrodynamics

2000

We have generalised the exact solution of the Riemann problem in special relativistic hydrodynamics for arbitrary tangential flow velocities. The solution is obtained by solving the jump conditions across shocks plus an ordinary differential equation arising from the self-similarity condition along rarefaction waves, in a similar way as in purely normal flow. The dependence of the solution on the tangential velocities is analysed, and the impact of this result on the development of multidimensional relativistic hydrodynamic codes (of Godunov type) is discussed.

PhysicsShock waveDifferential equationMechanical EngineeringMathematical analysisAstrophysics (astro-ph)Zero (complex analysis)Fluid Dynamics (physics.flu-dyn)FOS: Physical sciencesPhysics - Fluid DynamicsCondensed Matter PhysicsAstrophysicssymbols.namesakeExact solutions in general relativityRiemann problemFlow velocityMechanics of MaterialsOrdinary differential equationsymbolsJump
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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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Baseband modulation instability as the origin of rogue waves

2015

International audience; We study the existence and properties of rogue-wave solutions in different nonlinear wave evolution models that are commonly used in optics and hydrodynamics. In particular, we consider the Fokas-Lenells equation, the defocusing vector nonlinear Schrödinger equation, and the long-wave-shortwave resonance equation. We show that rogue-wave solutions in all of these models exist in the subset of parameters where modulation instability is present if and only if the unstable sideband spectrum also contains cw or zero-frequency perturbations as a limiting case (baseband instability). We numerically confirm that rogue waves may only be excited from a weakly perturbed cw whe…

Physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]SidebandNonlinear Sciences - Exactly Solvable and Integrable SystemsFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesModulation; stability; baseband-modulationPattern Formation and Solitons (nlin.PS)Physics - Fluid DynamicsResonance (particle physics)InstabilityNonlinear Sciences - Pattern Formation and SolitonsAtomic and Molecular Physics and OpticsNonlinear systemModulational instabilityClassical mechanicsNonlinear Sciences::Exactly Solvable and Integrable Systems[NLIN.NLIN-PS]Nonlinear Sciences [physics]/Pattern Formation and Solitons [nlin.PS]ModulationBasebandRogue waveExactly Solvable and Integrable Systems (nlin.SI)Nonlinear Sciences::Pattern Formation and SolitonsOptics (physics.optics)Physics - Optics
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Complex singularities and PDEs

2015

In this paper we give a review on the computational methods used to capture and characterize the complex singularities developed by some relevant PDEs. We begin by reviewing the classical singularity tracking method and give an example of application using the Burgers equation as a case study. This method is based on the analysis of the Fourier spectrum of the solution and it allows to determine and characterize the complex singularity closest to the real domain. We then introduce other methods generally used to detect the hidden singularities. In particular we show some applications of the Padé approximation, of the Kida method, and of Borel-Polya method. We apply these techniques to the s…

Physics::Fluid DynamicsComplex singularity Fourier transforms Padé approximation Borel and power series methods dispersive shocks fluid mechanics zero viscosity.Fluid Dynamics (physics.flu-dyn)FOS: Physical sciencesMathematical Physics (math-ph)Physics - Fluid DynamicsMathematical Physics
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Analysis of complex singularities in high-Reynolds-number Navier-Stokes solutions

2013

AbstractNumerical solutions of the laminar Prandtl boundary-layer and Navier–Stokes equations are considered for the case of the two-dimensional uniform flow past an impulsively-started circular cylinder. The various viscous–inviscid interactions that occur during the unsteady separation process are investigated by applying complex singularity analysis to the wall shear and streamwise velocity component of the two solutions. This is carried out using two different methodologies, namely a singularity-tracking method and the Padé approximation. It is shown how the van Dommelen and Shen singularity that occurs in solutions of the Prandtl boundary-layer equations evolves in the complex plane be…

Prandtl numberMathematics::Analysis of PDEsFOS: Physical sciencesPhysics::Fluid Dynamicssymbols.namesakeFlow separationSingularityboundary layer separation Navier–Stokes equations transition to turbulenceFOS: MathematicsMathematics - Numerical AnalysisComplex Variables (math.CV)Navier–Stokes equationsSettore MAT/07 - Fisica MatematicaMathematical PhysicsPhysicsMathematics - Complex VariablesMechanical EngineeringMathematical analysisFluid Dynamics (physics.flu-dyn)Reynolds numberLaminar flowPhysics - Fluid DynamicsMathematical Physics (math-ph)Numerical Analysis (math.NA)Condensed Matter PhysicsMechanics of MaterialssymbolsGravitational singularityPotential flow
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