Insight into the halogen-bond nature of noble gas-chlorine systems by molecular beam scattering experiments, Ab initio calculations and charge displacement analysis

Francesca Nunzi*, Diego Cesario, Leonardo Belpassi, Francesco Tarantelli, Luiz F. Roncaratti, Stefano Falcinelli, David Cappelletti, Fernando Pirani

*Corresponding author for this work

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

We have carried out molecular-beam scattering experiments and high-level ab initio investigations on the potential energy surfaces of a series of noble-gas-Cl 2 adducts. This effort has permitted the construction of a simple, reliable and easily generalizable analytical model potential formulation, which is based on a few physically meaningful parameters of the interacting partners and transparently shows the origin, strength, and stereospecificity of the various interaction components. The results demonstrate quantitatively beyond doubt that the interaction between a noble-gas (Ng) atom-even He-and Cl 2 in a collinear configuration is characterized by weak halogen bond (XB) formation, accompanied by charge transfer (CT) from the Ng to chlorine. This characteristic, which stabilizes the adduct, rapidly disappears on going towards the T-shaped configuration, dominated by pure van der Waals (vdW) forces. Similarly, a pure vdW interaction takes place-with no CT component in any configuration-if Cl 2 is present in the lowest π g ∗ → σ u ∗ excited state, because the change in electron density that accompanies the excitation eliminates the Cl 2 polar flattening and σ hole, making the XB interaction inaccessible.

Original languageEnglish
Pages (from-to)7330-7340
Number of pages11
JournalPhysical Chemistry Chemical Physics
Volume21
Issue number14
Early online date11 Mar 2019
DOIs
Publication statusPublished - 14 Apr 2019

Funding

F. N., D. C., F. T., and F. P. thank the MIUR and the Universita’ degli Studi di Perugia for financial support to the project AMIS, through the program ‘‘Dipartimenti di Eccellenza – 2018–2022’’. F. P. acknowledges funding from the MIUR (Ministero dell’Istru-zione, dell’Universitàe della Ricerca) in the framework of research project PRIN 2015 ‘‘STARS in the CAOS-Simulation Tools for Astrochemical Reactivity and Spectroscopy in the Cyberinfras-tructure for Astrochemical Organic Species’’, No. 2015F59J3R. We dedicated this paper to the memory of Gerardo Delgado-Barrio for his outstanding contribution to this field.

FundersFunder number
Ministero dell’Istru-zione, dell’Universitàe della Ricerca2015F59J3R
Ministero dell’Istruzione, dell’Università e della Ricerca
Università degli Studi di Perugia

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