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Motion of a spherical solid particle in thermal counterflow turbulence
Author(s) -
Demosthenes Kivotides
Publication year - 2008
Publication title -
physical review b
Language(s) - English
Resource type - Journals
eISSN - 1538-4489
pISSN - 1098-0121
DOI - 10.1103/physrevb.77.174508
Subject(s) - vortex , physics , turbulence , mechanics , magnetosphere particle motion , particle (ecology) , classical mechanics , thermal velocity , drag , collision frequency , stratification (seeds) , flow velocity , flow (mathematics) , plasma , quantum mechanics , oceanography , magnetic field , geology , seed dormancy , germination , botany , dormancy , biology
With numerical methods, we formulate and solve a mathematical model of solid-particle motion in thermal counterflow turbulence. We find a direct link between the intensity of vortex-particle collision induced Kelvin waves (vortex-gas ``temperature'') and the intensity of the particle-velocity fluctuations around its mean value. The latter mean value is determined by three factors: (a) the frequency of head-on particle-vortex collisions, (b) the formation of a vortex-tail behind the particle, and (c) the viscous drag. The frequency of head-on particle-vortex collisions depends on (a) the vortex line density, (b) the average tangle drift relative to the particle, and (c) the degree of tangle stratification normal to the counterflow direction. A higher stratification degree reduces the frequency of head-on collisions and allows the vortex-tail effect to dominate. At $T=1.3\text{K}$, vortex voids in the tangle act like barriers to particle motion; the particle-velocity fluctuations are comparable to its mean value and, thus, the particle's direction of motion is sporadically reversed.

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