Structure determination of formic acid reaction products on TiO2(110)

被引:75
作者
Sayago, DI
Polcik, M
Lindsay, R
Toomes, RL
Hoeft, JT
Kittel, M
Woodruff, DP [1 ]
机构
[1] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
[2] Univ Manchester, Nanosci Res Ctr, Manchester M13 9PL, Lancs, England
[3] Univ Manchester, Dept Chem, Manchester M13 9PL, Lancs, England
[4] Max Planck Gesell, Fritz Haber Inst, D-14195 Berlin, Germany
[5] Daresbury Lab, CCLRC, Warrington WA4 4AD, Cheshire, England
关键词
D O I
10.1021/jp049833s
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Using chemical-state-specific scanned-energy-mode photoelectron diffraction (PhD) from O 1s and C 1s photoemission, we have determined the local structure of the surface species produced on the rutile TiO2(110) surface as a result of room temperature exposure to formic acid. The results show clear evidence for the coexistence of formate, HCOO, and hydroxyl, OH, surface species. The formate species is aligned along [001], bridging an adjacent pair of surface 5-fold-coordinated Ti atoms with the formate O atoms nearly atop the Ti atoms with a Ti-O bond length of 2.08 +/- 0.03 Angstrom, consistent with scanning tunneling microscopy observations, a number of theoretical calculations, and an earlier very restricted PhD study. The hydroxyl species are formed by H attachment to the surface bridging O atoms and have a Ti-O bond length of 2.02 +/- 0.05 Angstrom, significantly longer than for the bridging oxygen atoms on a bulk-terminated surface or as previously reported for the clean surface. Our results exclude the possibility of a large (1/3) fractional occupation by the formate species of a second site azimuthally rotated by 90degrees and bonded to a surface oxygen vacancy site, as proposed in some earlier infrared and X-ray absorption spectroscopic studies. A much smaller concentration of such a second species cannot be excluded.
引用
收藏
页码:14316 / 14323
页数:8
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