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首页> 外文期刊>Applied Surface Science >CZTS absorber layer for thin film solar cells from electrodeposited metallic stacked precursors (Zn/Cu-Sn)
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CZTS absorber layer for thin film solar cells from electrodeposited metallic stacked precursors (Zn/Cu-Sn)

机译:用于电沉积金属堆叠前驱体(Zn / Cu-Sn)的薄膜太阳能电池的CZTS吸收层

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摘要

In the present work, Kesterite-Cu2ZnSnS4 (CZTS) thin films were successfully synthesized from stacked bilayer precursor (Zn/Cu-Sn) through electrodeposition-annealing route. Adherent and homogeneous Cu-poor, Zn-rich stacked metal Cu-Zn-Sn precursors with different compositions were sequentially electrodeposited, in the order of Zn/Cu-Sn onto Mo foil substrates. Subsequently, stacked layers were soft annealed at 350 degrees C for 20 min in flowing N-2 atmosphere in order to improve intermixing of the elements. Then, sulfurization was completed at 585 degrees C for 15 min in elemental sulfur environment in a quartz tube furnace with N-2 atmosphere. Morphological, compositional and structural properties of the films were investigated using SEM, EDS and XRD methods. Raman spectroscopy with two different excitation lines (514.5 and 785 nm), has been carried out on the sulfurized films in order to fully characterize the CZTS phase. Higher excitation wavelength showed more secondary phases, but with low intensities. Glow discharge optical emission spectroscopy (GDOES) has also been performed on films showing well formed Kesterite CZTS along the film thickness as compositions of the elements do not change along the thickness. In order to investigate the electronic structure of the CZTS, Photoluminescence (PL) spectroscopy has been carried out on the films, whose results matched up with the literatures. (C) 2016 Elsevier B.V. All rights reserved.
机译:在目前的工作中,成功地从堆叠的双层前驱体(Zn / Cu-Sn)通过电沉积退火路线合成了Kesterite-Cu2ZnSnS4(CZTS)薄膜。将具有不同组成的附着均匀的贫铜,富锌堆叠金属Cu-Zn-Sn前体按Zn / Cu-Sn的顺序依次电沉积到Mo箔基板上。随后,将堆叠的层在流动的N-2气氛中在350摄氏度下软退火20分钟,以改善元素的混合。然后,在具有N-2气氛的石英管炉中在元素硫环境中在585℃下进行15分钟的硫化。使用SEM,EDS和XRD方法研究了薄膜的形貌,组成和结构特性。为了完全表征CZTS相,已在硫化膜上进行了两种不同激发线(514.5和785 nm)的拉曼光谱分析。较高的激发波长显示出更多的次级相,但强度较低。辉光放电发射光谱法(GDOES)也已在显示出沿膜厚形成良好的Kesterite CZTS的膜上进行,因为元素的组成沿厚度不变。为了研究CZTS的电子结构,对薄膜进行了光致发光(PL)光谱分析,其结果与文献相吻合。 (C)2016 Elsevier B.V.保留所有权利。

著录项

  • 来源
    《Applied Surface Science》 |2016年第30期|91-97|共7页
  • 作者单位

    Politecn Milan, Dipartimento Chim Mat & Ingn Chim Giulio Natta, Via Mancinelli 7, I-20131 Milan, Italy;

    Politecn Milan, Dipartimento Chim Mat & Ingn Chim Giulio Natta, Via Mancinelli 7, I-20131 Milan, Italy;

    Politecn Milan, Dipartimento Chim Mat & Ingn Chim Giulio Natta, Piazza Leonardo da Vinci 32, I-20133 Milan, Italy;

    Univ Milano Bicocca, Dept Mat Sci, Via Cozzi 53, I-20125 Milan, Italy|Univ Milano Bicocca, Solar Energy Res Ctr MIB SOLAR, Via Cozzi 53, I-20125 Milan, Italy;

    Univ Milano Bicocca, Dept Mat Sci, Via Cozzi 53, I-20125 Milan, Italy|Univ Milano Bicocca, Solar Energy Res Ctr MIB SOLAR, Via Cozzi 53, I-20125 Milan, Italy;

    Politecn Milan, Dipartimento Chim Mat & Ingn Chim Giulio Natta, Via Mancinelli 7, I-20131 Milan, Italy;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Kesterite; CZTS; Bilayer precursor; Sulfurization; Photoluminescence etc;

    机译:钾长石;CZTS;双层前驱体;硫化;光致发光等;

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