Royal Society of Chemistry, Physical Chemistry Chemical Physics, 8(20), p. 5553-5568, 2018
DOI: 10.1039/c7cp05966c
Full text: Unavailable
Using an off-lattice kinetic Monte Carlo model we reproduce experimental laboratory trends in the density of amorphous solid water (ASW) for varied deposition angle, rate and surface temperature. Extrapolation of the model to conditions appropriate to protoplanetary disks and interstellar dark clouds indicate that these ices may be less porous than laboratory ices.