Flocculation of suspended cohesive particles in homogeneous isotropic turbulence
arXiv:2105.11735 · doi:10.1017/jfm.2021.487
Abstract
We investigate the dynamics of cohesive particles in homogeneous isotropic turbulence, based on one-way coupled simulations that include Stokes drag, lubrication, cohesive and direct contact forces. We observe a transient flocculation phase characterized by a growing average floc size, followed by a statistically steady equilibrium phase. We analyze the temporal evolution of floc size and shape due to aggregation, breakage, and deformation. Larger turbulent shear and weaker cohesive forces yield elongated flocs that are smaller in size. Flocculation proceeds most rapidly when the fluid and particle time scales are balanced and a suitably defined Stokes number is \textit{O}(1). During the transient stage, cohesive forces of intermediate strength produce flocs of the largest size, as they are strong enough to cause aggregation, but not so strong as to pull the floc into a compact shape. Small Stokes numbers and weak turbulence delay the onset of the equilibrium stage. During equilibrium, stronger cohesive forces yield flocs of larger size. The equilibrium floc size distribution exhibits a preferred size that depends on the cohesive number. We observe that flocs are generally elongated by turbulent stresses before breakage. Flocs of size close to the Kolmogorov length scale preferentially align themselves with the intermediate strain direction and the vorticity vector. Flocs of smaller size tend to align themselves with the extensional strain direction. More generally, flocs are aligned with the strongest Lagrangian stretching direction. The Kolmogorov scale is seen to limit floc growth. We propose a new flocculation model with a variable fractal dimension that predicts the temporal evolution of the floc size and shape.
arXiv commentaccepted for publication in the Journal of Fluid Mechanics
References in corpus (12)
- Dust coagulation and fragmentation in molecular clouds. I. How collisions between dust aggregates alter the dust size distribution
- Dust coagulation in protoplanetary disks: porosity matters
- Collision model for fully-resolved simulations of flows laden with finite-size particles
- A collision model for grain-resolving simulations of flows over dense, mobile, polydisperse granular sediment beds
- Alignment of vorticity and rods with Lagrangian fluid stretching in turbulence
- Settling of cohesive sediment: particle-resolved simulations
- On the clustering of finite-size particles in turbulence
- Forcing homogeneous turbulence in DNS of particulate flow with interface resolution and gravity
- Collisions between equal sized ice grain agglomerates
- Tetrahedron deformation and alignment of perceived vorticity and strain in a turbulent flow
- Collision-induced breakage of agglomerates in homogenous isotropic turbulence laden with adhesive particles
- An efficient cellular flow model for cohesive particle flocculation in turbulence