pith. sign in

arxiv: 1705.04778 · v1 · pith:LJWIPTR7new · submitted 2017-05-13 · 🌌 astro-ph.EP · cond-mat.soft

Collisions between sintered icy aggregates

classification 🌌 astro-ph.EP cond-mat.soft
keywords aggregatescollisionalgrowthnecksinteringaggregatecollisionsresults
0
0 comments X
read the original abstract

Collisions between sintered icy dust aggregates are numerically simulated. If the temperature of an icy aggregate is sufficiently high, sintering promotes molecular transport and a neck between adjacent grains grows. This growth changes the mechanical responses of the neck. We included this effect to a simulation code, and conducted collisional simulations. For porous aggregates, the critical velocity for growth, below which the mass of an aggregate increases, decreased from 50\,m\,s$^{-1}$ for the non-sintered case to 20\,m\,s$^{-1}$. For compacted aggregates, the main collisional outcome is bouncing. These results come from the fact that the strength of the neck is increased by sintering. The numerical results suggest that the collisional growth of icy grain aggregates is strongly affected by sintering.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A semi-analytic model of the bouncing barrier for protoplanetary dust aggregates

    astro-ph.EP 2026-06 unverdicted novelty 6.0

    A semi-analytic model using elastoplastic contact mechanics and weakest-link fracture statistics reproduces the sticking-bouncing boundary from DEM simulations and places the bouncing barrier within ALMA-inferred size...