化学
扩展X射线吸收精细结构
氧烷
催化作用
X射线吸收精细结构
星团(航天器)
氢
丙烷
离子
无机化学
反应速率
选择性催化还原
吸收(声学)
结晶学
吸收光谱法
光谱学
材料科学
有机化学
物理
复合材料
量子力学
计算机科学
程序设计语言
作者
Junji Shibata,Ken‐ichi Shimizu,Yuu Takada,Akira Shichi,Hisao Yoshida,Shigeo Satokawa,Atsushi Satsuma,Tadashi Hattori
标识
DOI:10.1016/j.jcat.2004.08.007
摘要
The detailed structure of Ag clusters formed in H zeolites during H2 reduction as well as under NO + C3H8 + O2 + H2 reaction condition is examined with H2-TPR, XRD, UV–vis, and Ag K-edge XAFS. H2-TPR results suggest a quantitative conversion of the exchanged Ag+ ion to Ag2pp+ cluster in Ag-MFI during H2 reduction in a temperature range from 373 to 573 K. Combined with the UV–vis spectrum of the cluster, exhibiting bands at 255 and 305 nm, and Ag K-edge EXAFS result, the structure of the cluster is identified as Ag42+. UV–vis and Ag K-edge XANES/EXAFS results reveal that, during NO + C3H8 + O2 + H2 reaction at 573 K, part of the Ag+ ions are converted to Agnδ+ clusters, whose average structure can be close to Ag42+. The amount of the clusters increases with the Ag/Al ratio of Ag zeolites. The NO reduction rate of Ag-MFI for the NO + C3H8 + O2 reaction is significantly improved by an addition of 0.5% H2, and the rate increases with Ag/Al ratio of Ag-MFI. This cluster does not form on Ag-MOR under the same conditions, and the NO reduction rate does not increase by H2 addition. The structure–activity relationship shows that the Agnδ+, probably the Ag42+ cluster, in Ag-MFI catalysts is responsible for the selective reduction of NO by C3H8.
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