Electronic Structures of Late versus Early Transition Metal Imido Complexes from 15N-NMR Signatures

被引:0
作者
Kakiuchi, Yuya [1 ]
Coperet, Christophe [1 ]
机构
[1] Swiss Fed Inst Technol, Dept Chem & Appl Biosci, Vladimir Prelog Weg 1-5, CH-8093 Zurich, Switzerland
基金
瑞士国家科学基金会;
关键词
Imido complex; N-15 NMR spectroscopy; solid-state NMR; electronic structure; ORDER REGULAR APPROXIMATION; NUCLEAR-MAGNETIC-RESONANCE; SPIN-STATE ENERGETICS; NMR CHEMICAL-SHIFTS; SHIELDING TENSORS; COBALT(III) IMIDO; REACTIVITY; BOND; NICKEL; CARBENE;
D O I
10.1002/hlca.202400142
中图分类号
O6 [化学];
学科分类号
0703 ;
摘要
Imido ligand is a ubiquitous motif in organometallic chemistry, serving roles spanning from ancillary ligands to reactive sites. The nature of M=N bond is highly depended on the metal centres and their d-electron configuration, with late transition metal (TM) imido complexes exhibiting contrasting features when compared to their early TM analogues. Envisioning to uncover general electronic descriptor for the nature of imido ligands, we computationally investigate the solid-state 15N NMR signatures of late TM imido complexes with various central metals, geometries and d-electron counts, and compare them against these of the corresponding early TM systems. The spectroscopic signatures are mostly driven by the presence of filled, pi-symmetry orbitals in late TM imido complexes, suggesting the development of high-lying pi(M=N) and low-lying sigma/sigma*(M=N) orbitals. This contrasts with what is observed for the reported early TM systems, for which high-lying sigma-type orbitals determine the NMR signature. Noteworthily, Ni- and Pd-imido complexes with formal d10 configurations exhibit highly asymmetric nitrogen-15 NMR signature with extremely deshielded principal components, because of the presence of filled, high-lying antibonding pi*(M=N) orbitals, consistent with their high reactivity. The sensitive response of 15N NMR signature to the nature of metal sites further highlights that chemical shift is a useful reactivity descriptor.
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页数:10
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