The first well-defined Mo oxido-alkylidene complex, [(tBu3PN)2Mo(O)(CHSiMe3)] (4), and its borane adduct, [(tBu3PN)2Mo(O–B(C6F5)3)(CHSiMe3)] (5), have been prepared through alkylation of the bis(phosphinimide) Mo oxido-dichlorido complex [(tBu3PN)2MoOCl2] (3). The reaction between 2 equiv of tBu3PN–SiMe3 (2) and [(DME)MoO2Cl2] (1) generates 3 through selective elimination of (Me3Si)2O. All complexes have been studied in solution by multinuclear NMR spectroscopy and in the solid state by X-ray crystallography. Preliminary ROMP catalysis results are also presented.
Direct photochemical reduction of CO(2) has generally been accomplished by using transition-metal compounds as electron transfer reagents. Here, we show that elemental bromine can function as an alternative photosensitizer. When sunlight is tightly focused on mixtures of CO(2) and Br(2), in the presence of a polar adsorbent such as silica gel, glass wool, alumina, or titania, a metastable red adduct is formed within seconds and concentrates at the point of illumination. Further illumination causes deposition of a stable black film on the polar adsorbent. Mass spectrometry of the cold-trapped red intermediate shows clusters of peaks corresponding to the expected distribution of isotopomers of C(2)O(4)Br(4)(+), as well as of C(2)O(4)Br(3)(+). DFT computations indicate that the lowest-energy species with the formula C(2)O(4)Br(4) is trans-2,4-dibromo-2,4-dihypobromo-1,3-dioxetane. Formation of this molecule from (2CO(2) + 2Br(2)) would require a minimum of 3 visible photons, two of which would hypothetically be used in formation of as-yet undetected CO(2)Br(2) and the third, in a subsequent photodimerization. By elemental analysis, the final amorphous solid product contains a C/Br atomic ratio >12, suggesting that Br(2) is acting photocatalytically. Even with a poorly optimized optical system, the reaction rate has reached as high as 1.6 mg reduced C with 40 s of solar collection using a 30 cm diameter paraboloid reflector. This rate is consistent with the storage of approximately 1% of incident solar energy.
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