The role of interstitial sites in the Ti3d defect state in the band gap of Titania

被引:803
作者
Wendt, Stefan [1 ]
Sprunger, Phillip T. [1 ,2 ]
Lira, Estephania [1 ]
Madsen, Georg K. H. [1 ]
Li, Zheshen [1 ]
Hansen, Jonas O. [1 ]
Matthiesen, Jesper [1 ]
Blekinge-Rasmussen, Asger [1 ]
Laegsgaard, Erik [1 ]
Hammer, Bjork [1 ]
Besenbacher, Flemming [1 ]
机构
[1] Aarhus Univ, Interdisciplinary Nanosci Ctr iNANO, Dept Phys & Astron, DK-8000 Aarhus C, Denmark
[2] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70808 USA
关键词
D O I
10.1126/science.1159846
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Titanium dioxide ( TiO2) has a number of uses in catalysis, photochemistry, and sensing that are linked to the reducibility of the oxide. Usually, bridging oxygen ( O-br) vacancies are assumed to cause the Ti3d defect state in the band gap of rutile TiO2( 110). From high- resolution scanning tunneling microscopy and photoelectron spectroscopy measurements, we propose that Ti interstitials in the near- surface region may be largely responsible for the defect state in the band gap. We argue that these donor- specific sites play a key role in and may dictate the ensuing surface chemistry, such as providing the electronic charge required for O-2 adsorption and dissociation. Specifically, we identified a second O-2 dissociation channel that occurs within the Ti troughs in addition to the O-2 dissociation channel in O-br vacancies. Comprehensive density functional theory calculations support these experimental observations.
引用
收藏
页码:1755 / 1759
页数:5
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