Homoleptic Organocobalt(III) Compounds with Intermediate Spin
Homoleptic organocobalt(III) compounds with formula [NBu4][CoIII(C6X5)4] [X = F (3), Cl (4)] were obtained in reasonable yields by chemical oxidation of the corresponding divalent species [NBu4]2[CoII(C6X5)4] [X = F (1), Cl (2)]. The [CoIII(C6X5)4]−/[CoII(C6X5)4]2– couples are electrochemically r...
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Veröffentlicht in: | Inorganic chemistry 2014-12, Vol.53 (23), p.12384-12395 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | Homoleptic organocobalt(III) compounds with formula [NBu4][CoIII(C6X5)4] [X = F (3), Cl (4)] were obtained in reasonable yields by chemical oxidation of the corresponding divalent species [NBu4]2[CoII(C6X5)4] [X = F (1), Cl (2)]. The [CoIII(C6X5)4]−/[CoII(C6X5)4]2– couples are electrochemically related by quasi-reversible, one-electron exchange processes at moderate potential: E 1/2 = −0.29 (X = F) and −0.36 V (X = Cl) versus saturated calomel electrode. The [CoIII(C6X5)4]− anions in salts 3 and 4 show an unusual square-planar geometry as established by single-crystal X-ray diffraction methods. According to their stereochemistry, these CoIII derivatives (d6) are paramagnetic non-Kramers systems with a large zero-field splitting contribution and no observable electron paramagnetic resonance (EPR) spectrum. The thermal dependence of their magnetic susceptibilities can be explained in terms of a spin-Hamiltonian formalism with S = 1 ground state (intermediate spin) and substantial spin–orbit contribution. The magnetic properties of the square-planar d7 parent species [NBu4]2[CoII(C6X5)4] were also thoroughly studied both at microscopic (EPR) and macroscopic levels (alternating current and direct current magnetization measurements). They behave as S = 1/2 (low spin) systems with mainly (d z 2 )1 electron configuration and a certain degree of s-orbital admixture that has been quantified. The electronic structures of all four open-shell [Co(C6X5)4] q− compounds (q = 1, 2) accounting for their respective magnetic properties are based on a common orbital energy-level diagram. |
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ISSN: | 0020-1669 1520-510X |
DOI: | 10.1021/ic501719y |