On the elastoplastic behavior in collisional compression of spherical dust aggregates
arXiv:2408.15573 · doi:10.1007/s10035-024-01463-x
Abstract
Aggregates consisting of submicron-sized cohesive dust grains are ubiquitous, and understanding the collisional behavior of dust aggregates is essential. It is known that low-speed collisions of dust aggregates result in either sticking or bouncing, and local and permanent compaction occurs near the contact area upon collision. In this study, we perform numerical simulations of collisions between two aggregates and investigate their compressive behavior. We find that the maximum compression length is proportional to the radius of aggregates and increases with the collision velocity. We also reveal that a theoretical model of contact between two elastoplastic spheres successfully reproduces the size- and velocity-dependence of the maximum compression length observed in our numerical simulations. Our findings on the plastic deformation of aggregates during collisional compression provide a clue to understanding the collisional growth process of aggregates.
22 pages, 15 figures. Accepted for publication in Granular Matter
References in corpus (9)
- The Physics of Protoplanetesimal Dust Agglomerates. IV. Towards a Dynamical Collision Model
- The Physics of Protoplanetesimal Dust Agglomerates II. Low Velocity Collision Properties
- Tensile Strength of Porous Dust Aggregates
- Fractal aggregates of sub-micron-sized grains in the young planet-forming disk around IM Lup
- Compression Behaviour of Porous Dust Agglomerates
- Experimental study on compression property of regolith analogues
- The Physics of Protoplanetesimal Dust Agglomerates. X. Mechanical properties of dust aggregates probed by a solid-projectile impact
- Thermal conductivity and coordination number of compressed dust aggregates
- Threshold velocity for collisional growth of porous dust aggregates consisting of cohesive frictionless spheres