An Approach to Estimate the Binding energy of Interstellar Species
Ankan Das, Milan Sil, Prasanta Gorai, Sandip K. Chakrabarti and, Jean-Christophe Loison

TL;DR
This study systematically calculates the binding energies of interstellar species on water ice clusters, improving accuracy by increasing cluster size and comparing results with experimental data to better model interstellar chemistry.
Contribution
It introduces a method using water cluster models of increasing size to more accurately estimate binding energies of astrochemical species on water ice.
Findings
Binding energies converge with larger water clusters.
Water c-pentamer and hexamer models yield results close to experimental values.
The approach enhances modeling of interstellar chemical processes.
Abstract
One of the major obstacles to accurately model the interstellar chemistry is an inadequate knowledge about the binding energy (BE) of interstellar species with dust grains. In denser region of molecular cloud, where very complex chemistry is active, interstellar dust is predominantly covered by H2O molecules and thus it is essential to know the interaction of gas phase species with water ice to trace realistic physical and chemical processes. To this effect, we consider water (cluster) ice to calculate the BE of several atoms, molecules, and radicals of astrochemical interest. Systematic studies have been carried out to come up with a relatively more accurate BE of astrophysically relevant species on water ice. We increase the size of the water cluster methodically to capture the realistic situation. Sequentially one, three, four, five and six water molecules are considered to represent…
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