The enhanced conductivity and stability of AZO thin films with a TiO2 buffer layer

Aluminum doped zinc oxide (AZO) films were substitutes of the SnO2:F films on soda lime glass substrate in the amorphous thin-film solar cells due to good properties and low cost. In order to improve properties of AZO films, the TiO2 buffer layer had been introduced. AZO films with and without TiO2...

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Published inPhysica. B, Condensed matter Vol. 407; no. 23; pp. 4518 - 4522
Main Authors Yang, Tianlin, Song, Shumei, Li, Yanhui, Xin, Yanqing, Du, Guiqiang, Lv, Maoshui, Han, Shenghao
Format Journal Article
LanguageEnglish
Published Kidlington Elsevier B.V 01.12.2012
Elsevier
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Summary:Aluminum doped zinc oxide (AZO) films were substitutes of the SnO2:F films on soda lime glass substrate in the amorphous thin-film solar cells due to good properties and low cost. In order to improve properties of AZO films, the TiO2 buffer layer had been introduced. AZO films with and without TiO2 buffer layer were deposited on soda lime glass substrates by r.f. magnetron sputtering. Subsequently, one group samples were annealed in vacuum (0.1Pa) at 500°C for 120s using the RTA system, and the influence of TiO2 thickness on the properties of AZO films had been discussed. The XRD measurement results showed that all the films had a preferentially oriented (002) peak, and the intensity of (002) peak had been enhanced for the AZO films with TiO2 buffer layer. The resistivity of TiO2 (3.0nm)/AZO double-layer film is 4.76×10−4Ωcm with the maximum figure merit of 1.92×10−2Ω−1, and the resistivity has a remarkable 28.7% decrease comparing with that of the single AZO film. The carrier scattering mechanism of TiO2 (3.0nm)/AZO double-layer film had been described by Hall measurement in different temperatures. The average transmittance of all the films exceeded 92% in the visible spectrum. Another group samples were heat treated in the quartz tube in air atmosphere, and the effect of TiO2 thickness on thermal stability of AZO films had been discussed.
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content type line 23
ISSN:0921-4526
1873-2135
DOI:10.1016/j.physb.2012.08.015