On the growth process of Cu 2 ZnSn(S,Se) 4 absorber layer formed by selenizing CuZnSSnS precursors and its photovoltaic performance Jianjun Li a , Yi Zhang a,n , Hongxia Wang b , Li Wu c , Jiguo Wang a , Wei Liu a , Zhiqiang Zhou a , Qing He a , Yun Sun a,n a Institute of Photoelectronic Thin Film Devices and Technology and Tianjin Key Laboratory of Thin Film Devices and Technology, Nankai University, Tianjin 300071, PR China b School of Chemistry, Physics and Mechanical Engineering, Science and Engineering Faculty, Queensland University of Technology, Brisbane, QLD 4001, Australia c The MOE Key Laboratory of Weak-Light Nonlinear Photonics, School of Physics, Nankai University, Tianjin 300071, PR China article info Article history: Received 5 February 2014 Received in revised form 31 July 2014 Accepted 5 September 2014 Keywords: CZTSSe Stacking order Growth properties Selenization Solar cell abstract Sputtering and subsequent sulfurization (or selenization) is one of the methods that have been extensively employed to fabricate Cu 2 ZnSn(S,Se) 4 (CZTSSe) thin lms. However, there are limited reports on the effect of precursor stacking order of the sputtered source materials on the properties of the synthesized CZTSSe lms. In this work, the morphology and crystallization process of the CZTSSe lms which were prepared by selenizing CuZnSSnS precursor layers with different stacking sequences and the adhesion property between the as-synthesized CZTSSe layer and Mo substrate have been thoroughly investigated. It has been found that the growth of CZTSSe material and the morphology of the lm strongly depend on the location of Cu layer in the precursor lm. The formation of CZTSSe starts from the diffusion of CuSe to Sn(S,Se) layer to form CuSn(S,Se) compound, followed by the reaction with Zn(S,Se). The investigation of the morphology of the CZTSSe lms has shown that large grains are formed in the lm with the precursor stacking order of Mo/SnS/ZnS/Cu, which is attributed to a bottom-to-top growth mechanism. In contrast, the lm made from a precursor with a stacking sequence of Mo/ZnS/ SnS/Cu is mainly consisted of small grains due to a top-to-bottom growth mechanism. The best CZTSSe solar cell with energy conversion efciency of 3.35% has been achieved with the selenized Mo/ZnS/ SnS/Cu lm, which is attributed to a good contact between the absorber layer and the Mo substrate. & 2014 Elsevier B.V. All rights reserved. 1. Introduction The rare, thus high cost of In and Ga elements which are used in Cu(In,Ga)Se 2 (CIGS) based light absorbing material [1,2] has recently raised signicant concern on the production scale of CIGS based thin lm solar cells. To solve this issue, a substitute material based on Cu 2 ZnSn(S,Se) 4 (CZTSSe) which uses earth-abundant, thus much cheaper elements Zn and Sn to replace In and Ga in CIGS has received considerable attention since 2009 [3,4]. CZTSSe is derived from CIGS compound and normally adopts kesterite or stannite structure [5,6]. Fundamentally speaking, CZTSSe has a desirable optoelectronic prop- erty for PVs including an optimal band gap of 1.01.5 eV [68] depending on the ratio of Se/S [9], and a high absorption coefcient larger than 10 4 cm À1 [5,7,9] in visible spectrum range. In practice, CZTSSe lm can be made using the approaches that have been applied in CIGS lm fabrication, such as co-evaporation, sputtering combined with post-sulfurization or selenization, electro-deposition, spin-coating combined with subsequent annealing, and so on [3,4]. Among them, sputtering is one of the promising methods which are viable for large-scale production of CZTSSe thin lms. In sputtering deposition, variable combination of target sources based on either metal or binary metal suldes have been used to make the precursor for CZTSSe lm [1014]. Katagiri et al. have reported CZTSSe solar cells with power conversion efciency of 6.77% which were made by co- sputtering Cu, ZnS and SnS precursor [15]. Chawl and Clemens have further improved the power conversion efciency of CZTSSe solar cells to 9.3% by co-sputtering Cu x (S,Se) y , Zn x (S,Se) y and Sn x (S,Se) y composites [16]. Since different stacking order of the sputtering source materials can be adopted for deposition of the precursor layers, it brings up the question of whether the different stacking order has any impact on the property of the synthesized light absorber material. Fernandes et al. have reported the synthesis of CZTS thin lms which were made by sulfurizing the sputtered metal precursors with the stacking order of Mo/Zn/Sn/Cu and Mo/Zn/Cu/Sn. They have found that the Contents lists available at ScienceDirect journal homepage: www.elsevier.com/locate/solmat Solar Energy Materials & Solar Cells http://dx.doi.org/10.1016/j.solmat.2014.09.023 0927-0248/& 2014 Elsevier B.V. All rights reserved. n Corresponding authors. Tel.: þ86 22 23508572 8018; fax: þ86 22 23508912. E-mail addresses: yizhang@nankai.edu.cn (Y. Zhang), suny@nankai.edu.cn (Y. Sun). Solar Energy Materials & Solar Cells 132 (2015) 363371