Ab initio Calculation of Binding Energies of Interstellar Sulphur-Containing Species on Crystalline Water Ice Models
Jessica Perrero, Albert Rimola, Marta Corno, Piero Ugliengo

TL;DR
This study uses ab initio methods to accurately calculate the binding energies of sulfur-containing molecules on water ice, aiding astrochemical models of interstellar environments.
Contribution
It introduces a cost-effective computational approach combining HF-3c and DFT for reliable binding energy predictions on crystalline water ice.
Findings
DFT B3LYP-D3(BJ) provides accurate binding energies.
HF-3c followed by DFT yields comparable results to full DFT calculations.
Computed binding energies agree well with literature data.
Abstract
There are different environments in the interstellar medium (ISM), depending on the density, temperature and chemical composition. Among them, molecular clouds, often referred to as the cradle of stars, are paradigmatic environments relative to the chemical diversity and complexity in space. Indeed, there, radio to far-infrared observations revealed the presence of several molecules in the gas phase, while near-infrared spectroscopy detected the existence of submicron sized dust grains covered by H2O -dominated ice mantles. The interaction between gas-phase species and the surfaces of water ices is measured by the binding energy (BE), a crucial parameter in astrochemical modelling. In this work, the BEs of a set of sulphur-containing species on water ice mantles have been computed by adopting a periodic ab initio approach using a crystalline surface model. The Density Functional Theory…
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