A contact model for sticking of adhesive meso-particles

Abstract

The interaction between visco-elasto-plastic and adhesive particles is the subject of this study, where "meso-particles" are introduced, i.e., simplified particles, whose contact mechanics is not taken into account in all details. A few examples of meso-particles include agglomerates or groups of primary particles, or inhomogeneous particles with micro-structures of the scale of the contact deformation, such as core-shell materials.A simple, flexible contact model for meso-particles is proposed, which allows to model the bulk behavior of assemblies of many particles in both rapid and slow, quasi-static flow situations. An attempt is made to categorize existing contact models for the normal force, discuss all the essential mechanical ingredients that must enter the model (qualitatively) and finally solve it analytically.The model combines a short-ranged, non-contact part (resembling either dry or wet materials) with an elaborate, visco-elasto-plastic and adhesive contact law. Using energy conservation arguments, an analytical expression for the coefficient of restitution is derived in terms of the impact velocity (for pair interactions or, equivalently, without loss of generality, for quasi-static situations in terms of the maximum overlap or confining stress).Adhesive particles (or meso-particles) stick to each other at very low impact velocity, while they rebound less dissipatively with increasing velocity, in agreement with previous studies. For even higher impact velocities an interesting second sticking and rebound regime is reported. The low velocity sticking is due to non-contact adhesive forces, the first rebound regime is due to stronger elastic and kinetic energies with little dissipation, while the high velocity sticking is generated by the non-linearly increasing, history dependent plastic dissipation and adhesive contact force. As the model allows also for a stiff, more elastic core material, this causes the second rebound regime at even higher velocities.

On super-elastic collisions between magnetized plasmoids in the heliosphere

“…Intuitively, we expect a large change in magnetic topology in case of merging, so that the occurrence of the latter depends on magnetic reconnection. Even if our understanding of reconnection in this large-S problem is still far from complete, a simple model (in analogy with elastoplastic collisions [64]) suggests that the choice between bouncing and merging depends on the relative velocity of the plasmoids. Indeed, the larger such velocity, the faster the change of magnetic flux, the larger the induced electric field and the corresponding dissipation, which is related to modifications of magnetic topology.…”

“…Again, the analogy with elastoplastic collisions -see Fig. 6 in [64] -suggests that a dissipation-related criterion exists: if v C is below (above) a threshold v thr , then collisions lead to bouncing (merging). As for plasmoids, Fig.…”