Definition
In a microscopic Monte Carlo model, when used for grain chemistry, the positions of each atom or molecule on the grain mantle can be followed. Thus, for an ice mantle consisting of 50 monolayers, the approach will follow all of the atoms and molecules as well as unoccupied sites for each of the 50 monolayers. In the simplest approach, each monolayer is modeled as a rectangular grid of potential wells in lattice sites with or without occupation. The atoms or molecules move from lattice well to well and possibly react when they land in the same site, while the species in the outermost layer also desorb into the gas, as gas-phase species accrete onto the outermost monolayer. The choice of which process happens in which time period depends upon the approach utilized. In the continuous time random-walk approach, a kinetic Monte Carlo approach used most commonly in the astrochemical literature, a Poisson (or waiting time) distribution (ψa(t) = kaexp(−kat)) is used, where kais...
References and Further Reading
Chang Q, Herbst E (2016) Unified microscopic-macroscopic simulations of complex organic molecule chemistry in cold cores. Astrophys J 819:145 (13 pages)
Clements AR, Berk B, Cooke IR, Garrod RT (2018) Kinetic Monte Carlo simulations of water ice porosity: extrapolations of deposition parameters from the laboratory to interstellar space. Phys Chem Chem Phys 20:5553–5568
Vasyunin AI, Herbst E (2013) A unified Monte Carlo treatment of gas-grain chemistry for large reaction networks. II. A multiphase gas-surface-layered bulk model. Astrophys J 762:86 (21 pages)
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2018 Springer-Verlag GmbH Germany, part of Springer Nature
About this entry
Cite this entry
Herbst, E. (2018). Micro-Monte-Carlo Models. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_5389-1
Download citation
DOI: https://doi.org/10.1007/978-3-642-27833-4_5389-1
Received:
Accepted:
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-27833-4
Online ISBN: 978-3-642-27833-4
eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics