Issue 2, 2011

Gauging electronic dissymmetry in bis-chelates of titanium(iv) using sterically and electronically variable 2,2′-biphenoxides

Abstract

3,3′,5,5′-Tetrasubstituted-2,2′-biphenolate complexes of titanium(IV) with bis(diketonate) (Bob), bis(hydroxamate) (Hox) and mixed diketonate–hydroxamate (Hob) ligands have been prepared from the corresponding diisopropoxide complexes. Four of the twelve compounds have been characterized crystallographically, and in the solid state all show the (Δ,R)/(Λ,S) relative stereochemistry at titanium and the biaryloxide, respectively, as previously observed in (acac)2Ti(1,1′-bi-2-naphtholate) complexes. In solution the compounds epimerize by atropisomerization of the biphenolate moiety with ΔG ≈ 14 kcal mol−1. The bis(diketonate) complexes show high diastereoselectivity except for the most electron-poor tetranitrobiphenolate. In contrast, the bis(hydroxamate) shows low to moderate selectivity which correlates with the steric but not electronic properties of the biphenolates (Br < CH3 < NO2 < tBu). The mixed diketonate–hydroxamate complexes show intermediate behaviour. These observations are rationalized on the basis of MO arguments regarding ligand-metal π bonding. Symmetrical chelates such as diketonates foster mixing of two dπ orbitals and create a dissymmetric electronic environment. This mixing does not take place with unsymmetrical ligands such as hydroxamates, which therefore do not create an environment where electronic effects contribute significantly to binding stereoselectivity.

Graphical abstract: Gauging electronic dissymmetry in bis-chelates of titanium(iv) using sterically and electronically variable 2,2′-biphenoxides

Supplementary files

Article information

Article type
Edge Article
Submitted
04 Sep 2010
Accepted
07 Oct 2010
First published
27 Oct 2010

Chem. Sci., 2011,2, 331-336

Gauging electronic dissymmetry in bis-chelates of titanium(IV) using sterically and electronically variable 2,2′-biphenoxides

N. Kongprakaiwoot, M. Quiroz-Guzman, A. G. Oliver and S. N. Brown, Chem. Sci., 2011, 2, 331 DOI: 10.1039/C0SC00468E

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