On the master equation approach to diffusive grain-surface chemistry: the H, O, CO system

T. Stantcheva; V. I. Shematovich; E. Herbst

doi:10.1051/0004-6361:20020838

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arXiv · astro-ph/0306545

On the master equation approach to diffusive grain-surface chemistry: the H, O, CO system

T. Stantcheva·V. I. Shematovich·E. Herbst

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Abstract

We have used the master equation approach to study a moderately complex network of diffusive reactions occurring on the surfaces of interstellar dust particles. This network is meant to apply to dense clouds in which a large portion of the gas-phase carbon has already been converted to carbon monoxide. Hydrogen atoms, oxygen atoms, and CO molecules are allowed to accrete onto dust particles and their chemistry is followed. The stable molecules produced are oxygen, hydrogen, water, carbon dioxide (CO2), formaldehyde (H2CO), and methanol (CH3OH). The surface abundances calculated via the master equation approach are in good agreement with those obtained via a Monte Carlo method but can differ considerably from those obtained with standard rate equations.

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T. Stantcheva, V. I. Shematovich, E. Herbst. 2003-06-26. On the master equation approach to diffusive grain-surface chemistry: the H, O, CO system. https://doi.org/10.1051/0004-6361%3A20020838

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