H067-03
Mesh-Free numerical simulation of swarm transport and evolution in fractured media
Abstract:
Numerical simulations track a swarm of particles that mutually interact through their (inertia-less) Stokeslets fields while settling under gravity. An accelerated summation scheme drastically reduces computation below O(N2) operations. Wall effects in various fracture geometries are modeled using the method of fundamental solutions (MFS). To support quantitative comparison of the results with previous experiments, the initial injection process is also modeled with suitable wall effects, and experimental parameters of the swarm and fractures are incorporated into the simulations.
The simulations demonstrate that the fundamental phenomena observed during experiments (tail formation, breakup, and bifurcation of a swarm) can be explained within the realm of Stokes flow. Results also reveal how strongly the ultimate breakup depends upon the early swarm shape, which is affected by details of the injection process and wall effects. Breakup of the swarm reduces its settling speed, so time/distance to breakup is an important quantity for the efficiency of transport of subsurface particulates. Directions of future research will be discussed, including multi-scale porous spaces and polydisperse swarms.
Acknowledgment: This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Geosciences Research Program under Award Number (DE-FG02-09ER16022).