Phase evolution of Cu2ZnSnS4 (CZTS) kesterite thin films during the sulfurization process

被引:37
作者
Jung, Hyo Rim [1 ]
Shin, Seung Wook [2 ]
Gurav, K. V. [1 ]
Suryawanshi, M. P. [3 ]
Hong, Chang Woo [1 ]
Yang, Han Seung [1 ]
Lee, Jeong Yong [2 ]
Moon, Jong Ha [1 ]
Kim, Jin Hyeok [1 ]
机构
[1] Chonnam Natl Univ, Optoelect Convergence Res Ctr, Dept Mat Sci & Engn, Kwangju 500757, South Korea
[2] Inst for Basic Sci Korea, Ctr Nanomat & Chem React, Taejon 305701, South Korea
[3] Shivaji Univ, Thin Film Mat Lab, Dept Phys, Kolhapur 416004, Maharashtra, India
基金
新加坡国家研究基金会;
关键词
Cu2ZnSnS4 (CZTS); Thin film solar cells (TFSCs); Phase evolution; Transmission electron microscopy (TEM); Earth abundant elements; RAMAN-SCATTERING; ATMOSPHERE; TIME;
D O I
10.1016/j.ceramint.2015.06.145
中图分类号
TQ174 [陶瓷工业]; TB3 [工程材料学];
学科分类号
0805 ; 080502 ;
摘要
The development of high efficiency Cu2ZnSnS4 (CZTS) thin film solar cells depends on the synthesis of phase pure CZTS films. Due to the narrow phase window, it is difficult to prepare CZTS films with a pure kesterite phase (i.e., a film that lacks traces of detrimental secondary phases). For this, phase evolution of kesterite CZTS in films must be systematically studied. In the present study detailed phase evolution of kesterite CZTS via the sulfurization of stacked Cu/SnS2/ZnS precursor was examined. The phase evolution of kesterite CZTS was analyzed during the temperature-dependent sulfurization of stacked precursors. In addition to traditional X-ray diffraction and Raman analysis, transmission electron microscopy (TEM) characterization was used to study the phase evolution and trace locations of secondary phases in the sulfurized films. Furthermore, based on the experimental evidences the reaction pathways for the formation of CZTS kesterite phase and plausible phase evolution mechanism are proposed. (C) 2015 Published by Elsevier Ltd and Techna Group S.r.l.
引用
收藏
页码:13006 / 13011
页数:6
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