Search results for "Turbulence"

showing 10 items of 378 documents

Phenomenological description of counterflow superfluid turbulence in rotating containers

2004

In this paper a simple equation for the vortex line density describing some of the most relevant observed effects in counterflow superfluid turbulence in ${}^{4}\mathrm{He}$ in the presence of rotation is proposed. This model is based on a generalization of Vinen's equation which incorporates as additional quantity the angular velocity \ensuremath{\Omega}.

PhysicsCondensed Matter::OtherGeneralizationTurbulenceAngular velocityCondensed Matter PhysicsRotationOmegaElectronic Optical and Magnetic MaterialsVortexSuperfluidityClassical mechanicsLine (formation)Mathematical physics
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Alternative Vinen equation and its extension to rotating counterflow superfluid turbulence

2007

Two alternative Vinen's evolution equations for the vortex line density L in counterflow superfluid turbulence, are physically admissible and lead to analogous results in steady states. In Phys. Rev. B, 69, 094513 (2004) the most used of them was generalized to counterflow superfluid turbulence in rotating containers. Here, the analogous generalization for the alternative Vinen's equation is proposed. Both generalized Vinen's equations are compared with the experimental results, not only in steady-states but also in some unsteady situations. From this analysis follows that the solutions of the alternative Vinen's equation tend significantly faster to the corresponding final steady state val…

PhysicsCondensed Matter::OtherTurbulenceGeneralizationFOS: Physical sciencesTourbillonCondensed Matter PhysicsRotationSuperfluid turbulenceElectronic Optical and Magnetic MaterialsVortexCondensed Matter - Other Condensed MatterSuperfluidityVortex tangleClassical mechanicsRotating counterflow turbulenceLine (geometry)Electrical and Electronic EngineeringSettore MAT/07 - Fisica MatematicaSuperfluid helium-4Other Condensed Matter (cond-mat.other)Physica B: Condensed Matter
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Condensation of classical nonlinear waves

2005

We study the formation of a large-scale coherent structure (a condensate) in classical wave equations by considering the defocusing nonlinear Schr\"odinger equation as a representative model. We formulate a thermodynamic description of the condensation process by using a wave turbulence theory with ultraviolet cut-off. In 3 dimensions the equilibrium state undergoes a phase transition for sufficiently low energy density, while no transition occurs in 2 dimensions, in analogy with standard Bose-Einstein condensation in quantum systems. Numerical simulations show that the thermodynamic limit is reached for systems with $16^3$ computational modes and greater. On the basis of a modified wave tu…

PhysicsCondensed Matter::Quantum GasesPhase transitionStatistical Mechanics (cond-mat.stat-mech)Thermodynamic equilibriumWave turbulenceCondensationGeneral Physics and AstronomyFOS: Physical sciencesWave equationSchrödinger equationNonlinear systemsymbols.namesakeClassical mechanicssymbolsNonlinear Schrödinger equationCondensed Matter - Statistical Mechanics
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Observation of the kinetic condensation of classical waves

2012

International audience; The observation of Bose-Einstein condensation, in which particle interactions lead to a thermodynamic transition into a single, macroscopically populated coherent state, is a triumph of modern physics(1-5). It is commonly assumed that this transition is a quantum process, relying on quantum statistics, but recent studies in wave turbulence theory have suggested that classical waves with random phases can condense in a formally identical manner(6-9). In complete analogy with gas kinetics, particle velocities map to wavepacket k-vectors, collisions are mimicked by four-wave mixing, and entropy principles drive the system towards an equipartition of energy. Here, we use…

PhysicsCondensed Matter::Quantum GasesSPECTRUMDIGITAL HOLOGRAPHYCondensed Matter::OtherCondensationGeneral Physics and AstronomyWEAK-TURBULENCEKinetic energyPHOTONS01 natural sciencesTHERMALIZATION010305 fluids & plasmasCrystalNonlinear systemClassical mechanicsLIGHTGASQuantum mechanics0103 physical sciencesBOSE-EINSTEIN CONDENSATIONBose–Einstein condensationFIELD010306 general physicsQuantum
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Nonlocal effects in superfluid turbulence: Application to the low-density- to high-density-state transition and to vortex decay

2005

We discuss a phenomenological equation for the evolution of vortex tangle in counterflow superfluid turbulence, which takes into account the influence of the nonlocal effects, introducing into the original equation of Vinen two simple corrective terms dependent on a nonvanishing ratio between the average separation between vortex lines and the diameter of the channel. The equation allows one to describe, in relatively good agreement with experimental results, the two turbulent regimes present in counterflow superfluid turbulence and the transition between them. The decay rate of the vortex line density L, when the heat flux is suddenly turned off, is also investigated; due to the simplicity…

PhysicsCondensed matter physicsCondensed Matter::OtherTurbulenceQuantum vortexCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsVortexSuperfluidityHelium-4Heat fluxQuantum electrodynamicsPhenomenological modelIsotopes of heliumPhysical Review B
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Refrigeration of an Array of Cylindrical Nanosystems by Flowing Superfluid Helium

2016

We consider the refrigeration of an array of heat-dissipating cylindrical nanosystems as a simplified model of computer refrigeration. We explore the use of He II as cooling fluid, taking into account forced convection and heat conduction. The main conceptual and practical difficulties arise in the calculation of the effective thermal conductivity. Since He II does not follow Fourier’s law, the effective geometry-dependent conductivity must be extracted from a more general equation for heat transfer. Furthermore, we impose the restrictions that the maximum temperature along the array should be less than (Formula presented.) transition temperature and that quantum turbulence is avoided, in o…

PhysicsCondensed matter physicsQuantum turbulenceRefrigerationConductivityCondensed Matter PhysicsThermal conduction01 natural sciencesNanorefrigerationAtomic and Molecular Physics and Optics010305 fluids & plasmasForced convectionThermal conductivityThermal conductivity0103 physical sciencesHeat transferGeneral Materials ScienceSuperfluid helium010306 general physicsSettore MAT/07 - Fisica MatematicaSuperfluid helium-4Journal of Low Temperature Physics
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Effective thermal conductivity of helium II: from Landau to Gorter–Mellink regimes

2014

The size-dependent and flux-dependent effective thermal conductivity of narrow channels filled with He II is analyzed. The classical Landau evaluation of the effective thermal conductivity of quiescent He II is extended to describe the transition to fully turbulent regime, where the heat flux is proportional to the cubic root of the temperature gradient (Gorter–Mellink regime). To do so, we use an expression for the quantum vortex line density L in terms of the heat flux considering the influence of the walls. From it, and taking into account the friction force of normal component against the vortices, we compute the effective thermal conductivity as a function of the heat flux, and we disc…

PhysicsCondensed matter physicsTurbulenceApplied MathematicsGeneral MathematicsQuantum vortexGeneral Physics and Astronomychemistry.chemical_elementHeat transfer coefficientThermal conductionThermal diffusivityThermal conductivitychemistryHeat fluxThermal conductivity Liquid helium Quantum turbulence Micropores Quantized vorticesSettore MAT/07 - Fisica MatematicaHelium
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Contribution of the normal component to the thermal resistance of turbulent liquid helium

2015

Previous results for the velocity profile of the normal component of helium II in counterflow are used to evaluate the viscous contribution to the effective thermal resistance. It turns out that such a contribution becomes considerably higher than the usual Landau estimate, because in the presence of vortices, the velocity profile is appreciably different from the Poiseuille parabolic profile. Thus, a marked increase in the contribution of the normal component to the thermal resistance with respect to the viscous Landau estimate does not necessarily imply that the normal component is turbulent. Furthermore, we examine the influence of a possible slip flow along the walls when the radius of …

PhysicsCondensed matter physicsTurbulenceApplied MathematicsGeneral MathematicsThermal resistanceQuantum turbulenceGeneral Physics and AstronomyRadiusHagen–Poiseuille equationVortexPhysics::Fluid DynamicsThermal resistance – Superfluid helium – Quantum turbulence – Normal componentBoundary value problemSettore MAT/07 - Fisica MatematicaSuperfluid helium-4Zeitschrift für angewandte Mathematik und Physik
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Vortex diffusion and vortex-line hysteresis in radial quantum turbulence

2014

Abstract We study the influence of vortex diffusion on the evolution of inhomogeneous quantized vortex tangles. A simple hydrodynamical model to describe inhomogeneous counterflow superfluid turbulence is used. As an illustration, we obtain solutions for these effects in radial counterflow of helium II between two concentric cylinders at different temperatures. The vortex diffusion from the inner hotter cylinder to the outer colder cylinder increases the vortex length density everywhere as compared with the non-diffusive situation. The possibility of hysteresis in the vortex line density under cyclical variations of the heat flow is explored.

PhysicsCondensed matter physicsTurbulenceHysteresisVortex diffusionQuantum turbulenceStarting vortexCondensed Matter PhysicsQuantum turbulenceElectronic Optical and Magnetic MaterialsVortexVortex ringCondensed Matter::SuperconductivityVortex stretchingHorseshoe vortexQuantized vorticeBurgers vortexElectrical and Electronic EngineeringSettore MAT/07 - Fisica MatematicaPhysica B: Condensed Matter
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Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium

2021

Both simulations and observations have shown that turbulence is a pervasive phenomenon in cosmic scenarios, yet it is particularly difficult to model numerically due to its intrinsically multiscale character which demands high resolutions. Additionally, turbulence is tightly connected to the dynamical state and the formation history of galaxies and galaxy clusters, producing a diverse phenomenlogy which requires large samples of such structures to attain robust conclusions. In this work, we use an adaptive mesh refinement (AMR) cosmological simulation to explore the generation and dissipation of turbulence in galaxy clusters, in connection to its assembly history. We find that major mergers…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Accretion (meteorology)TurbulenceFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVorticityEnstrophyAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Vortex stretchingIntracluster mediumGalaxy clusterAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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