1996
DOI: 10.1021/om950913f
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CO2 Activation. 7. Formation of the Catalytically Active Intermediate in the Hydrogenation of Carbon Dioxide to Formic Acid Using the [{(COD)Rh(μ-H)}4]/Ph2P(CH2)4PPh2 Catalyst:  First Direct Observation of Hydride Migration from Rhodium to Coordinated 1,5-Cyclooctadiene

Abstract: The nature of the catalytically active intermediate formed in situ from the tetrameric cluster [{(COD)Rh(μ-H)}4] (COD = 1,5-cyclooctadiene; 1) and the bidentate phosphane Ph2P(CH2)4PPh2 (dppb) during hydrogenation of CO2 to formic acid was investigated. Kinetic measurements suggest the initial formation of a catalyst precursor that reacts with dihydrogen to give the actual active species. NMR spectroscopic investigations of the reaction of 1 with dppb in THF-d 8 reveal three phosphorus-containing products that… Show more

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Cited by 49 publications
(27 citation statements)
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“…This gives an order of magnitude for the dynamical correlation energy contributions introduced by the large scale CMRCI approach. One can thus conclude that except for the 2 3 state, which could be close to the 25 000 cm −1 limit, all other states are predicted to be significantly higher.…”
Section: Figmentioning
confidence: 84%
See 1 more Smart Citation
“…This gives an order of magnitude for the dynamical correlation energy contributions introduced by the large scale CMRCI approach. One can thus conclude that except for the 2 3 state, which could be close to the 25 000 cm −1 limit, all other states are predicted to be significantly higher.…”
Section: Figmentioning
confidence: 84%
“…Transition-metal-containing molecules are of importance as catalysts in organic and organometallic chemistry (1)(2)(3)(4)(5) and their spectroscopic studies provide insight into chemical bonding in simple metal-containing systems (6). Transition-metalcontaining species are also of astrophysical importance (7)(8)(9)(10).…”
Section: Introductionmentioning
confidence: 99%
“…These species are also of chemical importance, particularly in catalysis (2)(3)(4). Because of the high cosmic abundance of transition metal elements in stars, some diatomic species are also of astrophysical importance and several diatomic oxide and hydride molecules have been identified in the atmospheres of cool M-and S-type stars (5)(6)(7)(8)(9).…”
Section: Introductionmentioning
confidence: 99%
“…Typically, high-energy reaction partners such as hydrogen, unsaturated compounds, or strained cyclic molecules can be used to drive the chemical reactions towards low energy products (e.g., Refs. [20,[22][23][24]). Therefore, the overall energy balance and the primary source of energy used to generate the starting materials have to be carefully considered and critically evaluated to assess whether or not a given transformation has the potential to lead to a net reduction of the CO 2 footprint.…”
Section: Introductionmentioning
confidence: 99%