Published in

Royal Society of Chemistry, Physical Chemistry Chemical Physics, 8(20), p. 5553-5568, 2018

DOI: 10.1039/c7cp05966c

Links

Tools

Export citation

Search in Google Scholar

Kinetic Monte Carlo simulations of water ice porosity: extrapolations of deposition parameters from the laboratory to interstellar space

Journal article published in 2018 by Aspen R. Clements ORCID, Brandon Berk ORCID, Ilsa R. Cooke ORCID, Robin T. Garrod ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Orange circle
Postprint: archiving restricted
Red circle
Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

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.

Beta version