Astrochemistry: an open molecular science cloud approach to low temperature reactivity

Abstract

The appropriate formulation of low temperature rate coefficients values for use in modelling astrochemical systems is a typical test bed for the implementation of Open Molecular Science Cloud management tools for distributed calculation (or downloading), validation and re-use of Molecular Science knowledge. Here the case of an abstraction reaction forming a rather stable intermediate of interest for astrochemical studies is considered.