Universal Statistical Properties of Inertial-particle Trajectories in Three-dimensional, Homogeneous, Isotropic, Fluid Turbulence

preprint2014arXivOpen access

Abstract

We uncover universal statistical properties of the trajectories of heavy inertial particles in three-dimensional, statistically steady, homogeneous, and isotropic turbulent flows by extensive direct numerical simulations. We show that the probability distribution functions (PDFs) P(ϕ)P(ϕ), of the angle ϕϕ between the Eulerian velocity u{\bf u} and the particle velocity v{\bf v}, at this point and time, shows a power-law region in which P(ϕ)∼ϕ−γP(ϕ) \sim ϕ^{-γ}, with a new universal exponent γ≃4γ\simeq 4. Furthermore, the PDFs of the trajectory curvature κκ and modulus θθ of the torsion ϑ\vartheta have power-law tails that scale, respectively, as P(κ)∼κ−hκP(κ) \sim κ^{-h_κ}, as κ→∞κ\to \infty, and P(θ)∼θ−hθP(θ) \sim θ^{-h_θ}, as θ→∞θ\to \infty, with exponents hκ≃2.5h_κ\simeq 2.5 and hθ≃3h_θ\simeq 3 that are universal to the extent that they do not depend on the Stokes number St{\rm St} (given our error bars). We also show that γγ, hκh_κ and hθh_θ can be obtained by using simple stochastic models. We characterize the complexity of heavy-particle trajectories by the number NI(t,St)N_{\rm I}(t,{\rm St}) of points (up until time tt) at which ϑ\vartheta changes sign. We show that nI(St)≡lim⁡t→∞NI(t,St)t∼St−Δn_{\rm I}({\rm St}) \equiv \lim_{t\to\infty} \frac{N_{\rm I}(t,{\rm St})}{t} \sim {\rm St}^{-Δ}, with Δ≃0.4Δ\simeq 0.4 a universal exponent.

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