Tumbling of small axisymmetric particles in random and turbulent flows.
We analyze the tumbling of small nonspherical, axisymmetric particles in random and turbulent flows. We compute the orientational dynamics in terms of a perturbation expansion in the Kubo number, and obtain the tumbling rate in terms of Lagrangian correlation functions. These capture preferential sampling of the fluid gradients, which in turn can give rise to differences in the tumbling rates of disks and rods. We show that this is a weak effect in Gaussian random flows. But in turbulent flows persistent regions of high vorticity cause disks to tumble much faster than rods, as observed in direct numerical simulations [S. Parsa, E. Calzavarini, F. Toschi, and G. A. Voth, Phys. Rev. Lett. 109, 134501 (2012)]. For larger particles (at finite Stokes numbers), rotational and translational inertia affects the tumbling rate and the angle at which particles collide, due to the formation of rotational caustics.
Department of Physics, Gothenburg University, 41296 Gothenburg, Sweden.
K
K
Gustavsson
Department of Physics, Gothenburg University, 41296 Gothenburg, Sweden.
J
J
Einarsson
Department of Physics, Gothenburg University, 41296 Gothenburg, Sweden.
B
B
Mehlig