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Chaotic Fluid Mixing in Crystalline Sphere Arrays

Abstract : We study the Lagrangian dynamics of steady 3D Stokes flow over simple cubic (SC) and body-centered cubic (BCC) lattices of close-packed spheres, and uncover the mechanisms governing chaotic mixing. Due to the cusp-shaped sphere contacts, the topology of the skin friction field is fundamentally different to that of continuous (non-granular) media (e.g. open pore networks), with significant implications for fluid mixing. Weak symmetry breaking of the flow orientation with respect to the lattice symmetries imparts a transition from regular to strong chaotic mixing in the BCC lattice, whereas the SC lattice only exhibits weak mixing. Whilst the SC and BCC lattices share the same symmetry point group, these differences are explained in terms of their space groups, and we find that a glide symmetry of the BCC lattice generates chaotic mixing. These insight are used to develop accurate predictions of the Lyapunov exponent distribution over the parameter space of mean flow orientation, and point to a general theory of mixing and dispersion based upon the inherent symmetries of arbitrary crystalline structures.
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https://hal-insu.archives-ouvertes.fr/insu-01731764
Contributor : Isabelle Dubigeon <>
Submitted on : Wednesday, March 14, 2018 - 2:26:10 PM
Last modification on : Tuesday, December 10, 2019 - 1:44:03 PM

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  • HAL Id : insu-01731764, version 1

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Régis Turuban, Daniel Lester, Tanguy Le Borgne, Yves Méheust. Chaotic Fluid Mixing in Crystalline Sphere Arrays . American Geophysical Union Fall Meeting 2017, Dec 2017, New Orleans, United States. pp.H31M-03. ⟨insu-01731764⟩

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