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

Author:

Clements Aspen R.1234ORCID,Berk Brandon1234ORCID,Cooke Ilsa R.1234ORCID,Garrod Robin T.12345ORCID

Affiliation:

1. Department of Chemistry

2. University of Virginia

3. Charlottesville

4. USA

5. Department of Astronomy

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.

Funder

National Aeronautics and Space Administration

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Reference48 articles.

1. Interstellar Ice: The Infrared Space Observatory Legacy

2. THESPITZERICE LEGACY: ICE EVOLUTION FROM CORES TO PROTOSTARS

3. The infrared spectra of amorphous solid water and ice Ic between 10 and 140 K

4. A. G. G. M. Tielens and L. J.Allamandola , Composition, structure, and chemistry of interstellar dust , National Aeronautics and Space Administration Technical Report , 1987

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