2000
DOI: 10.1021/ic000178m
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On the Failure To Observe Isotropic Electron Paramagnetic Resonance Spectra for Certain Chromium(I) Carbonyl Complexes

Abstract: Although isotropic EPR spectra have often been reported for Cr(I) complexes with degenerate ground states and consequent Jahn−Teller distortions, such spectra have not been reported for cis-dicarbonyl or fac-tricarbonyl complexes of Cr(I). The most likely explanation is that ground states are subject to an approximate accidental degeneracy, probably modulated by a ligand bending vibrational mode, thus providing an efficient spin−lattice relaxation pathway.

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Cited by 5 publications
(8 citation statements)
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“…S1) were simulated by a mixture of the three species using the spin Hamiltonian parameters given in table S1. Two of the room temperature spectra were in agreement with the previously reported species A (labeled A) with two magnetically equivalent 31 P nuclei (nuclear spin, I = ½ and isotropic hyperfine coupling, P A iso = 52.3 MHz) resulting in a 1:2:1 triplet (indicated by dashed lines in green) and Cr I -bisarene with 10 near-equivalent protons ( 1 H; I = ½; H A iso = 9.5 MHz) resulting in an undecet with 11 superhyperfine lines (with a binomial intensity distribution of 1:10:45:120:210:252:210:120:45: 20:1), with the exception of the two outer lines being too weak to be observed. 53 Cr (I = 3/2; natural abundance, 9.5%; Cr A iso = 50.5 MHz) causes quartet satellites where the undecet is further split into a 1:1:1:1 quartet.…”
Section: Resultssupporting
confidence: 89%
See 1 more Smart Citation
“…S1) were simulated by a mixture of the three species using the spin Hamiltonian parameters given in table S1. Two of the room temperature spectra were in agreement with the previously reported species A (labeled A) with two magnetically equivalent 31 P nuclei (nuclear spin, I = ½ and isotropic hyperfine coupling, P A iso = 52.3 MHz) resulting in a 1:2:1 triplet (indicated by dashed lines in green) and Cr I -bisarene with 10 near-equivalent protons ( 1 H; I = ½; H A iso = 9.5 MHz) resulting in an undecet with 11 superhyperfine lines (with a binomial intensity distribution of 1:10:45:120:210:252:210:120:45: 20:1), with the exception of the two outer lines being too weak to be observed. 53 Cr (I = 3/2; natural abundance, 9.5%; Cr A iso = 50.5 MHz) causes quartet satellites where the undecet is further split into a 1:1:1:1 quartet.…”
Section: Resultssupporting
confidence: 89%
“…A iso = 50.5 MHz), (b) X ( 13 CO) 0 (two 31 P and eight 1 H nuclei), (c) X ( 13 CO) 1 (two 31 P, eight 1 H, and one 13 C nuclei), (d) X ( 13 CO) 2 (two 31 P, eight 1 H, and two 13 C nuclei), (e) d 8 -X ( 13 CO) 0 (two 31 P and eight 2 H nuclei), (f) d 8 -X ( 13 CO) 1 (two 31 P, eight 2 H, and one 13 C nuclei), and (g) d 8 -X ( 13 CO) 2 (two 31 P, eight 2 H, and two 13 C nuclei). Additional spin Hamiltonian parameters: g iso = 1.9970; 31…”
Section: Sample Preparationmentioning
confidence: 99%
“…Although the EPR spectrum of [Cr(CO) 6 ] + has only once been reportedly observed at 4 K, 23 Bond et al gave a very comprehensive explanation on the failure to observe isotropic EPR signals for such a species. 24 Therefore, if [Cr(CO) 6 ] + is indeed formed, it would prove exceedingly difficult to detect by conventional X-band EPR. All attempts to detect [Cr(CO) 6 ] + in our experiments by EPR, and additionally by chemical oxidation of [Cr(CO) 6 ] with Ag[Al(OC(CF 3 ) 3 ) 4 ], proved to be unsuccessful, even at low temperatures (5 K).…”
Section: ■ Results and Discussionmentioning
confidence: 99%
“…One possible explanation is that [Cr­(CO) 6 ] + is formed during the photochemical transformation of [Cr­(CO) 4 (dppp)] + into trans -[Cr­(CO) 2 (dppp) 2 ] + or that phosphine-free Cr­(I) ions are released into solution and not observed by EPR. Although the EPR spectrum of [Cr­(CO) 6 ] + has only once been reportedly observed at 4 K, Bond et al gave a very comprehensive explanation on the failure to observe isotropic EPR signals for such a species . Therefore, if [Cr­(CO) 6 ] + is indeed formed, it would prove exceedingly difficult to detect by conventional X-band EPR.…”
Section: Resultsmentioning
confidence: 99%
“…Several mysteries remained from the work of Bond and Colton. We have recently provided an explanation for the failure to observe isotropic EPR spectra of fac -[Cr(CO) 3 L 3 ] + or cis -[Cr(CO) 2 L 4 ] + , but there are still a number of unsolved problems related to the mechanisms of Cr(I) reactions.…”
Section: Introductionmentioning
confidence: 99%