Show simple item record

dc.creatorChang, Qiangen_US
dc.creatorHerbst, Ericen_US
dc.date.accessioned2013-07-16T21:43:10Z
dc.date.available2013-07-16T21:43:10Z
dc.date.issued2013en_US
dc.identifier2013-WF-03en_US
dc.identifier.urihttp://hdl.handle.net/1811/55468
dc.descriptionAuthor Institution: Department of Chemistry, University of Virginia, Charlottesville, Virginia, USA; Department of Chemistry, Physics and Astronomy, University of Virginia, Charlottesville, Virginia, USAen_US
dc.description.abstractResults of ice formation on interstelar grains by full microscopic-macroscopic Monte Carlo simulation of gas-grain chemistry in cold dense interstellar clouds are reported. Gas phase chemical kinetics is treated by macroscopic Monte Carlo approach while reactions on grain are treated by microscopic Monte Carlo simulation. More than 200 diffusive surface reactions are included in the simulation and we model how photons penetrate thick layers of species and photodissociate species. Ice mantle on grain surfaces gradually build up as species accrete fron gas phase and react on the grain surface. Photodissociated species are allowed to diffuse and react within ice mantle. Our results can be compared with observations.en_US
dc.language.isoenen_US
dc.publisherOhio State Universityen_US
dc.titleUNIFIED MICROSCOPIC-MACROSCOPIC MONTE CARLO SIMULATION OF ICE FORMATION ON INTERSTELLAR GRAINSen_US
dc.typeArticleen_US
dc.typeImageen_US
dc.typePresentationen_US


Files in this item

Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail

Items in Knowledge Bank are protected by copyright, with all rights reserved, unless otherwise indicated.

This item appears in the following Collection(s)

Show simple item record