Water-Gas Shift Reaction on a Highly Active Inverse CeOx/Cu(111) Catalyst: Unique Role of Ceria Nanoparticles
Water-Gas Shift Reaction on a Highly Active Inverse CeOx/Cu(111) Catalyst: Unique Role of Ceria Nanoparticles
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DOI:
10.1002/anie.200903918
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发表时间:
2009-01-01
影响因子:
16.6
通讯作者:
Hrbek, Jan
中科院分区:
文献类型:
--
作者:
Rodriguez, Jose A.;Graciani, Jesus;Hrbek, Jan
The water-gas shift (WGS, CO+ H2O! CO2+ H2) is an important reaction frequently used in the chemical industry for the production of clean H2.[1] Oxide-supported copper catalysts show significant water-gas shift activity but their performance is not fully understood and is highly dependent on the synthesis conditions or the nature of the oxide support.[1–4] Either metallic Cu or Cu+ cations have been proposed as active sites for the WGS.[1–8] In addition, the oxide support may not be a simple spectator and may play a direct role in the catalytic process.[1, 4, 9] Extended surfaces and nanoparticles of metallic copper are able to catalyze the WGS [3, 5, 6, 10, 11] and Cu (111) has become a benchmark surface for studying the WGS.[3, 5, 11–14] Specific rates, activation energies, and reaction orders are consistent with data reported for ZnO-supported Cu catalysts.[5, 13] The rate-limiting step for the WGS on Cu (111) seems to be the dissociation of water,[11–13] and it is affected by the presence of surface modifiers such as S, O, or Cs.[13] Herein, we investigate the WGS reaction on Cu (111) surfaces partially covered with ceria nanoparticles. Bulk ceria is a well known oxide support for WGS catalysts.[1, 4, 8, 9] The CeOx/Cu (111) system allows us to study in detail the role of the oxide in the catalytic process and, furthermore, catalysts with an inverse oxide/metal configuration have some advantages for practical applications.[15] Figure 1 shows images of scanning tunneling microscopy (STM) acquired after dosing Ce to Cu (111) at 650 K under an atmosphere of O2 (p% 5 10À7 Torr). The reaction of O2 with the Cu (111) substrate leads to formation of a layer of copper oxide which exhibits domains of different reconstructions of a Cu2O (111) surface.[16] On top of the layer of copper oxide, there are two types of ceria features. These features were not seen in blank experiments for the adsorption of O2 on Cu (111). In Figure 1, small islands of ceria (2–5 nm in size, CeOx-I) appear on the terraces of the copper substrate, whereas large islands of ceria (30–50 nm in size, triangular shape, CeOx-II) are embedded in the substrate step edges. Inside the large ceria islands, a moirØ pattern can be seen with a separation of approximately 5 nm in between the depressions. The large ceria islands have a morphology different from that seen for the two most stable surfaces of bulk ceria: CeO2 (111) and CeO2 (110). An analysis of the structure of these islands reveals that they essentially have a height of 0.31 nm, which is consistent with a single layer of cerium sandwiched in between two layers of oxygen.[17] An O-Ce-O-Cu (interface) stacking is likely. The oxide nanoparticles in CeOx/Cu (111) display a morphology quite different from that found before for the growth of ceria nanoparticles on a Au (111) substrate using the same deposition methodology.[17] In the CeOx/Au (111) systems there were only large oxide islands at the step edges and these were exposing the (111) face of bulk ceria.[17] The interactions of