The gold catalyzed aerobic oxidation of alcohols is currently of great interest for the following reasons: 1) biomass-derived alcohols are a promising, renewable organic feedstock; 2) they use cheap, green oxidants, such as molecular oxygen (air) ; and 3) gold catalysts show extraordinarily high activities under mild conditions. The mechanistic aspects of gold catalyzed oxidation reactions of CO, H2, and other small molecules have been extensively studied, but a generally accepted oxidation mechanism for alcohols under similar conditions has not yet been formulated (however, see references [7–10]). Notably, the efficient low-temperature (50–120 8C) gold catalyzed oxidation of alcohols is known to proceed only in the liquid phase during the course of a long-term batch reaction with high oxygen pressure or intensive O2 flow. [1–4] On the other hand, we recently found that metallic gold nanoparticles supported on TiO2 gave rise to “double peak” catalytic activity in the gasphase oxidation of ethanol to acetaldehyde. The temperature, at which the first peak of activity occurred, 120 8C, was unusually low for the gas-phase reaction of primary alcohols. In contrast, gold supported on Al2O3 and SiO2 showed more usual behaviors, which were analogous to the second peak activity of Au/TiO2 at temperatures above 200 8C. [11] To account for these results, we proposed that specific active oxygen species form on the Au/TiO2 surface under mild reaction conditions and suggested hydrogen as a probable cofactor in their generation. Indeed, H2 can be produced concurrently as a result of ethanol anaerobic dehydrogenation and can thus participate in catalytic activity. In the present work, our efforts were focused on the role of hydrogen in the catalytic activity of gold supported on TiO2, Al2O3, and SiO2 matrixes to provide insights into the different profiles of ethanol oxidation. For this purpose, the O2 isotope exchange technique was applied in order to estimate the relative activity of the surface oxygen species. Oxygen isotope exchange (OIE) is a very sensitive direct method for evaluating the reactivity of surface oxygen atoms, which is a subject of primary interest in heterogeneous oxidation catalysis. Usually, as in the case of metal oxides, OIE is observed at 220–700 8C, although some metal oxides induce OIE at low temperatures after calcination and cooling in a vacuum. A highly reactive oxygen species, so called aoxygen, is generated on the Fe-ZSM5 zeolite surface after treatment with N2O. These species readily oxidize organics (benzene, methane, etc.) as well as perform OIE at room temperature. A special but relevant case, although photoinduced, is the OIE over TiO2, which also occurs at room temperature due to the involvement of reactive oxygen species, probably O anion radicals. Notably, a correlation was found between the TiO2 activity for the photoinduced OIE and the oxidation of isobutane, methanol, and ethanol over TiO2 upon ultraviolet (UV) irradiation. Generally, in a heterophase system comprising molecular dioxygen (O2) in the gas phase and oxygen on the surface of a solid (O), two isotope exchange reactions take place: 1) the hetero-exchange reaction [Equation (1)] , which is conveniently monitored by a fraction of the O isotope in the gas phase (a), and 2) the homo-exchange reaction [Equation (2)] , which is monitored by the parameter y = *C34 C34 (the difference between the equilibrium (*C34) and the current (C34) values for the fraction of asymmetric isotopic OO molecules). Obviously, the low-temperature activity of a catalyst in an oxygen homoexchange can indicate the involvement of very active surface oxygen species by analogy with the cases of a-oxygen and illuminated TiO2. [17]
Read full abstract