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  5. A “non-magnetic” triplet bismuthinidene enabled by relativity

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Preprint
English
2022

A “non-magnetic” triplet bismuthinidene enabled by relativity

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English
2022
DOI: 10.26434/chemrxiv-2022-d3jl7

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Frank Neese
Frank Neese

Max Planck

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Yue Pang
Nils Nöthling
Markus Leutzsch
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Abstract

Isolation and stabilization of main group diradical species have posed a synthetic challenge over the years due to their intrinsic high reactivity. Herein we report on a large-scale synthesis and isolation of a mono-coordinate bismuthinidene featuring a rigid and bulky ligand, which protects the Bi(I) center. The compound was characterized by its unique spectroscopic features (UV-vis and NMR), but more prominently, by its magnetic properties. Multiconfigurational quantum chemical calculations predict the ground state of the compound to be dominated by a spin-triplet. Further support for this electronic structure description was obtained through correlation of theory to experimental XRD, XAS, and UV-Vis data. However, all magnetic measurements (EPR, NMR and SQUID) point to a diamagnetic compound. This apparent discrepancy can be explained by an extremely large spin-orbit coupling (SOC) that leads to an unprecedented zero-field splitting of more than 8000 cm‒1, thus leaving a MS = 0 magnetic sublevel thermally isolated in the electronic ground state. The extremely large SOC effect is a result of the low-coordination number of the bismuth center in interplay with its heavy element nature.

How to cite this publication

Yue Pang, Nils Nöthling, Markus Leutzsch, Liqun Kang, Eckhard Bill, Maurice van Gastel, Edward J. Reijerse, Richard Goddard, Lucas Wagner, Daniel J. SantaLucia, Serena DeBeer, Frank Neese, Josep Cornellà (2022). A “non-magnetic” triplet bismuthinidene enabled by relativity. , DOI: 10.26434/chemrxiv-2022-d3jl7.

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Publication Details

Type

Preprint

Year

2022

Authors

13

Datasets

0

Total Files

0

Language

English

DOI

10.26434/chemrxiv-2022-d3jl7

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