論文

査読有り
2011年

UV irradiation effect on Al-doped anatase titanium dioxide

PHYSICA STATUS SOLIDI C: CURRENT TOPICS IN SOLID STATE PHYSICS, VOL 8, NO 1
  • Takao Sekiya
  • ,
  • Yasuhiro Takeda
  • ,
  • Shohei Ohya
  • ,
  • Tetsuya Kodaira

8
1
開始ページ
173
終了ページ
176
記述言語
英語
掲載種別
研究論文(国際会議プロシーディングス)
DOI
10.1002/pssc.201000663
出版者・発行元
WILEY-V C H VERLAG GMBH

Electron paramagnetic resonance (EPR) measurement under uv light irradiation was performed on Al-doped anatase TiO2 crystals grown by a chemical vapor transport method. In an as grown crystal, characteristic signals of EPR sextuplets are observed at 100-40 K. The intensity of the sextuplets decreases gradually with decreasing temperature. The sextuplets arise from a photogenerated hole of S=1/z interacting with an Al nuclear spin of I=5/2. The angular dependence of the sextuplets is successfully explained by a model where four symmetrically equivalent paramagnetic species giving the sextuplets are present in the crystal and the principal z-axis of a diagonal g-matrix for the paramagnetic species has a small deviation from the crystalline c-axis. The analysis of the angular dependence of the sextuplets gives anisotropic g-values of g(xx)=2.0254, g(yy)=2.0016, and g(zz)=2.0129, and hyperfine coupling constants of A(xx)=4.93, A(yy)=6.04, and A(zz)=5.98 G. An EPR signal from bulk Ti3+ is also observed at temperatures below 40 K regardless of uv irradiation. In an annealed crystal, the sextuplets are observed at temperatures below 70 K under uv irradiation. The EPR signal corresponding to bulk Ti3+ is absent in the entire temperature range. These experimental results differ greatly from those for the as-grown crystal. (c) 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

リンク情報
DOI
https://doi.org/10.1002/pssc.201000663
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000301525500037&DestApp=WOS_CPL
ID情報
  • DOI : 10.1002/pssc.201000663
  • ISSN : 1862-6351
  • Web of Science ID : WOS:000301525500037

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