Search results for "VISCOSITY"

showing 10 items of 542 documents

Ab initiosimulations of accretion disc instability

2003

We show that accretion disks, both in the subcritical and supercritical accretion rate regime, may exhibit significant amplitude luminosity oscillations. The luminosity time behavior has been obtained by performing a set of time-dependent 2D SPH simulations of accretion disks with different values of alpha and accretion rate. In this study, to avoid any influence of the initial disk configuration, we produced the disks injecting matter from an outer edge far from the central object. The period of oscillations is 2 - 50 s respectively for the two cases, and the variation amplitude of the disc luminosity is 10^38 - 10^39 erg/s. An explanation of this luminosity behavior is proposed in terms o…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)black hole physicsAb initioFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadiationAstrophysicsaccretion discsInstabilityLuminosityViscosityAmplitudeaccretionRadiation pressureinstabilitiesSpace and Planetary ScienceLimit cyclehydrodynamicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Numerical Simulations of the Thermal Instability Collapse in Radiation Pressure Dominated Disks

2005

We show that accretion disks, both in the subcritical and supercritical accretion rate regime, may exhibit significant amplitude luminosity oscillations. The luminosity time behavior has been obtained by performing a set of time‐dependent 2D SPH simulations of accretion disks with different values of α and accretion rate. An explanation of this luminosity behavior is proposed in terms of limit‐cycle instability: the disk oscillates between a radiation pressure dominated configuration (with a high luminosity value) and a gas pressure dominated one (with a low luminosity value). The origin of this instability is the difference between the heat produced by viscosity and the energy emitted as r…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadiationInstabilityLuminosityViscosityAmplitudeRadiation pressureMagnetorotational instabilityAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysics
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Nonlinear Critical Layers in Barotropic Stability

1991

Abstract Applying the method of matched asymptotic expansions (MAE) to the shallow water equations on a rotating sphere, the structure of critical layers that occur in the linear and inviscid analysis of neutral disturbances of barotropic zonal flows is investigated, assuming that the critical layers are controlled by nonlinearity rather than viscosity or nonparallel flow effects. It turns out that nonlinearity is insufficient to resolve the critical layer singularity completely. It suffices however to connect linear and nondissipative solutions across critical latitudes.

PhysicsAtmospheric Sciencebusiness.industryMechanicsMethod of matched asymptotic expansionsPhysics::Fluid DynamicsNonlinear systemViscositySingularityOpticsFlow (mathematics)Inviscid flowBarotropic fluidbusinessShallow water equationsPhysics::Atmospheric and Oceanic PhysicsJournal of the Atmospheric Sciences
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Critical Dynamics in a Binary Fluid: Simulations and Finite-Size Scaling

2006

We report comprehensive simulations of the critical dynamics of a symmetric binary Lennard-Jones mixture near its consolute point. The self-diffusion coefficient exhibits no detectable anomaly. The data for the shear viscosity and the mutual-diffusion coefficient are fully consistent with the asymptotic power laws and amplitudes predicted by renormalization-group and mode-coupling theories {\it provided} finite-size effects and the background contribution to the relevant Onsager coefficient are suitably accounted for. This resolves a controversy raised by recent molecular simulations.

PhysicsBinary fluidStatistical Mechanics (cond-mat.stat-mech)Shear viscosityDynamics (mechanics)FOS: Physical sciencesGeneral Physics and AstronomyBinary numberAmplitudePoint (geometry)Statistical physicsAnomaly (physics)ScalingCondensed Matter - Statistical MechanicsPhysical Review Letters
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Low compressibility accretion disc formation in close binaries: the role of physical viscosity

2006

Aims. Physical viscosity naturally hampers gas dynamics (rarefaction or compression). Such a role should support accretion disc development inside the primary gravitation potential well in a close binary system, even for low compressibility modelling. Therefore, from the astrophysical point of view, highly viscous accretion discs could exist even in the low compressibility regime showing strong thermal differences to high compressibility ones Methods. We performed simulations of stationary Smooth Particle Hydrodynamics (SPH) low compressibility accretion disc models for the same close binary system. Artificial viscosity operates in all models. The absence of physical viscosity and a superso…

PhysicsCauchy stress tensorAstronomy and AstrophysicsAstrophysicsPhysics::Fluid DynamicsSmoothed-particle hydrodynamicsViscosityClassical mechanicsSpace and Planetary ScienceInviscid flowMass transferCompressibilityViscous stress tensorNavier–Stokes equationsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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Computing bulk and shear viscosities from simulations of fluids with dissipative and stochastic interactions

2016

Exact values for bulk and shear viscosity are important to characterize a fluid and they are a necessary input for a continuum description. Here we present two novel methods to compute bulk viscosities by non-equilibrium molecular dynamics (NEMD) simulations of steady-state systems with periodic boundary conditions -- one based on frequent particle displacements and one based on the application of external bulk forces with an inhomogeneous force profile. In equilibrium simulations, viscosities can be determined from the stress tensor fluctuations via Green-Kubo relations; however, the correct incorporation of random and dissipative forces is not obvious. We discuss different expressions pro…

PhysicsCauchy stress tensorForce profileShear viscosityDissipative particle dynamicsGeneral Physics and AstronomyFOS: Physical sciences02 engineering and technologyMechanicsCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnology01 natural sciencesMolecular dynamicsShear (geology)0103 physical sciencesDissipative systemPeriodic boundary conditionsSoft Condensed Matter (cond-mat.soft)Physical and Theoretical Chemistry010306 general physics0210 nano-technology
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Methodisches zur bestimmung der viskositätszahl (staudinger-index) von cellulosen und cellulosenitraten

1959

An einem groseren Material von Cellulosenitraten wird die Konzentrationsabhangigkeit der spezifischen Viskositat im Hinblick auf die Reproduzierbarkeit der Einzelmessung und der Extrapolation nach c = 0 (bzw. ηsp = 0) untersucht. Es zeigt sich, das der eigent. liche Mesfehler, der im Mittel weniger als ± 2 % betragt, gelegentlich von einer erheblichen Inhomogenitat des Materials uberlagert wird. Als sicherstes Verfahren zur Bestimmung von [η] erwiest sich die Extrapolation der ηspc-Werte von mindestens vier Konzentrationen nach ηsp = 0, wobei ηsp far jede Konzentration aus vier Einzelmessungen gemittelt wird. Einfacher und annahernd von gleicher Genauigkeit ist die Berechung von [η] nach SC…

PhysicsConcentration dependenceIntrinsic viscosityPolymer chemistryAnalytical chemistryDie Makromolekulare Chemie
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Thermodynamic formalism for transport coefficients with an application to the shear modulus and shear viscosity.

2016

We discuss Onsager's thermodynamic formalism for transport coefficients and apply it to the calculation of the shear modulus and shear viscosity of a monodisperse system of repulsive particles. We focus on the concept of extensive "distance" and intensive "field" conjugated via a Fenchel-Legendre transform involving a thermodynamic(-like) potential, which allows to switch ensembles. Employing Brownian dynamics, we calculate both the shear modulus and the shear viscosity from strain fluctuations and show that they agree with direct calculations from strained and non-equilibrium simulations, respectively. We find a dependence of the fluctuations on the coupling strength to the strain reservoi…

PhysicsCoupling strengthStatistical Mechanics (cond-mat.stat-mech)Shear viscosityGeneral Physics and AstronomyFOS: Physical sciences02 engineering and technologyMechanics021001 nanoscience & nanotechnology01 natural sciencesShear modulusCondensed Matter::Soft Condensed MatterPhysics::Fluid DynamicsFormalism (philosophy of mathematics)0103 physical sciencesBrownian dynamicsPhysical and Theoretical Chemistry010306 general physics0210 nano-technologyCondensed Matter - Statistical MechanicsThe Journal of chemical physics
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Clustering and viscosity in a shear flow of a particulate suspension

2003

A shear flow of particulate suspension is analyzed for the qualitative effect of particle clustering on viscosity using a simple kinetic clustering model and direct numerical simulations. The clusters formed in a Couette flow can be divided into rotating chainlike clusters and layers of particles at the channel walls. The size distribution of the rotating clusters is scale invariant in the small-cluster regime and decreases rapidly above a characteristic length scale that diverges at a jamming transition. The behavior of the suspension can qualitatively be divided into three regimes. For particle Reynolds number Re(p) less than or approximately equal 0.1, viscosity is controlled by the char…

PhysicsDilatantReynolds numberThermodynamicsshearShear rateCondensed Matter::Soft Condensed MatterPhysics::Fluid DynamicsViscositysymbols.namesakeviscosityShear stresssymbolssuspensionsShear flowSuspension (vehicle)Couette flowflow shearshear properties
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On the Measurements of Numerical Viscosity and Resistivity in Eulerian MHD Codes

2016

We propose a simple ansatz for estimating the value of the numerical resistivity and the numerical viscosity of any Eulerian MHD code. We test this ansatz with the help of simulations of the propagation of (magneto)sonic waves, Alfven waves, and the tearing mode instability using the MHD code Aenus. By comparing the simu- lation results with analytical solutions of the resistive-viscous MHD equations and an empirical ansatz for the growth rate of tearing modes we measure the numerical viscosity and resistivity of Aenus. The comparison shows that the fast-magnetosonic speed and wavelength are the characteristic velocity and length, respectively, of the aforementioned (relatively simple) syst…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsEulerian pathMechanicsCharacteristic velocity01 natural sciencesNumerical resistivityRiemann solver010305 fluids & plasmassymbols.namesakeViscosityAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetorotational instability0103 physical sciencessymbolsMagnetohydrodynamicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)AnsatzThe Astrophysical Journal Supplement Series
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