Abstract

This article analyzes the nature of the chemical bond in coinage metal halides using high-level ab initio Valence Bond (VB) theory. It is shown that these bonds display a large Charge-Shift Bonding character, which is traced back to the large Pauli pressure arising from the interaction between the bond pair with the filled semicore d shell of the metal. The gold-halide bonds turn out to be pure Charge-Shift Bonds (CSBs), while the copper halides are polar-covalent bonds and silver halides borderline cases. Among the different halogens, the largest CSB character is found for fluorine, which experiences the largest Pauli pressure from its σ lone pair. Additionally, all these bonds display a secondary but non-negligible π bonding character, which is also quantified in the VB calculations.

Highlights

  • Understanding the nature of bonds in transition metal-containing molecules is a more challenging task than for main group atoms [1,2,3,4,5,6,7]

  • The detailed nature of bonding in coinage metal halide dimers has been dissected based on the high-level ab initio classical Valence Bond Breathing Orbital VB (BOVB) method

  • This method has been shown to provide accurate estimates of bond dissociation energies for these dimers, as compared with CCSD(T) combined with the large aug-cc-pVQZ basis set, and the bonding analysis inferred from the BOVB wave function can be considered as fully reliable and quantitative

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Summary

Introduction

Understanding the nature of bonds in transition metal-containing molecules is a more challenging task than for main group atoms [1,2,3,4,5,6,7]. A key reason is the presence of two different valence shells, the (n−1)d and ns shells, which have similar spatial extensions and energies These orbitals can be partially filled depending on the metal and its oxidation state and will usually involve a larger number of valence electrons than main group elements, which represent an additional complexity [8]. It is reasonable to expect that the presence of an electron-rich coinage metal M containing a filled (n−1)d semicore shell acting as lone pairs, together with a halogen X bearing lone pairs, can cause a significant CSB characteristics in the resulting MX dimers To tackle this bonding question, we apply, a high-level ab initio VB method. Two main issues are addressed in this article: quantifying the CSB character of MX, and dissecting the roles of the semicore fully filled (n−1)d shells in M atoms and of the lone pairs on X atoms in the bonding mechanism

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