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Chin. Phys. B, 2008, Vol. 17(6): 2170-2174    DOI: 10.1088/1674-1056/17/6/038
CLASSICAL AREAS OF PHENOMENOLOGY Prev   Next  

Enhanced optical nonlinear absorption of graded Au--TiO2 composite films

Liu Li(刘莉)a)b)† and Su Xiong-Rui(苏雄睿)b)
a College of Electronics & Information Engineering, Wuhan University of Science and Engineering, Wuhan 430073, China; b Department of Physics, Wuhan University, Wuhan 430072, China
Abstract  This paper reports that single-layer and graded Au--TiO2 granular composite films with Au atom content 15%--66% were prepared by using reactive co-sputtering technique. The third-order optical nonlinearity of single-layer and graded composite films was investigated by using s- and p-polarized Z-scans in femtosecond time scale. The nonlinear absorption coefficient βeff of single-layer Au--TiO2 films is measured to be --2.3×1030.76×103 cm/GW with Au atom content 15%--66%. The βeff value of the 10-layer Au--TiO2 graded film is enhanced to be --2.1×104cm/GW calculated from p-polarized Z-scans, which is about ten times the maximum βeff of single-layer films. Broadened response in the wavelength region 730--860 nm of the enhanced optical nonlinearity of graded Au--TiO2 composite films was also investigated.
Keywords:  Au--TiO2 granular composites      graded composite films      Z-scan      optical nonlinear absorption  
Received:  22 October 2007      Revised:  16 November 2007      Accepted manuscript online: 
PACS:  78.20.Ci (Optical constants (including refractive index, complex dielectric constant, absorption, reflection and transmission coefficients, emissivity))  
  42.65.An (Optical susceptibility, hyperpolarizability)  
  42.65.Re (Ultrafast processes; optical pulse generation and pulse compression)  
  78.66.-w (Optical properties of specific thin films)  
Fund: Project supported by the National Natural Science Foundation of China (Grant No 10474075).

Cite this article: 

Liu Li(刘莉) and Su Xiong-Rui(苏雄睿) Enhanced optical nonlinear absorption of graded Au--TiO2 composite films 2008 Chin. Phys. B 17 2170

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