Issue 3, 2025, Issue in Progress

Origin of 13C NMR chemical shifts elucidated based on molecular orbital theory: paramagnetic contributions from orbital-to-orbital transitions for the pre-α, α, β, α-X, β-X and ipso-X effects, along with effects from characteristic bonds and groups

Abstract

13 C NMR chemical shifts (δ(C)) were analysed via MO theory, together with the origin, using σd(C), σp(C) and σt(C), where C4− was selected as the standard for the analysis since σp(C: C4−) = 0 ppm. An excellent relationship was observed between σd(C) and the charges on C for (C4+, C2+, C0, C2− and C4−) and (C4−, CH22−, CH3 and CH4). However, such a relationship was not observed for the carbon species other than those above. The occupied-to-unoccupied orbital (ψiψa) transitions were mainly employed for the analysis. The origin was explained by the pre-α, α, β, α-X, β-X and ipso-X effects. The pre-α effect of an approximately 20 ppm downfield shift is theoretically predicted, and the observed α and β effects of approximately 10–15 ppm downfield shifts are well reproduced by the calculations, as are the variations in the α-X, β-X and ipso-X effects. Large downfield shifts caused by the formation of ethene (∼120 ppm), ethyne (∼60 ppm) and benzene (∼126 ppm) from ethane and carbonyl (∼146 ppm) and carboxyl (∼110 ppm) groups from CH3OH are also reproduced well by the calculations. The analysis and illustration of σp(C) through the ψiψa transitions enables us to visualize the effects and to understand the δ(C) values for the C atoms in the specific positions of the species. The occupied-to-occupied orbital (ψiψj) transitions are also examined. The theoretical investigations reproduce the observed results of δ(C). The origin for δ(C) and the mechanism are visualized, which allows us to image the process in principle. The role of C in the specific position of a compound in question can be more easily understood, which will aid in the development of highly functional compounds based on NMR.

Graphical abstract: Origin of 13C NMR chemical shifts elucidated based on molecular orbital theory: paramagnetic contributions from orbital-to-orbital transitions for the pre-α, α, β, α-X, β-X and ipso-X effects, along with effects from characteristic bonds and groups

Supplementary files

Article information

Article type
Paper
Submitted
18 Aug 2024
Accepted
06 Jan 2025
First published
21 Jan 2025
This article is Open Access
Creative Commons BY-NC license

RSC Adv., 2025,15, 1924-1940

Origin of 13C NMR chemical shifts elucidated based on molecular orbital theory: paramagnetic contributions from orbital-to-orbital transitions for the pre-α, α, β, α-X, β-X and ipso-X effects, along with effects from characteristic bonds and groups

W. Nakanishi, S. Hayashi and K. Matsuzaki, RSC Adv., 2025, 15, 1924 DOI: 10.1039/D4RA05980H

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