Faculty of Energy and Fuels, AGH University of Science and Technology, al. Mickiewicza 30, 30-059 Kraków, Poland.
Institute of Nuclear Physics, Polish Academy of Sciences, ul. Radzikowskiego 152, 31-342 Kraków, Poland.
Int J Mol Sci. 2023 Feb 5;24(4):3159. doi: 10.3390/ijms24043159.
We explore the important aspects of adventitious oxygen presence in nanopowders, as well as in the high-pressure and high-temperature-sintered nanoceramics of semiconductor kesterite CuZnSnS. The initial nanopowders were prepared via the mechanochemical synthesis route from two precursor systems, i.e., (i) a mixture of the constituent elements (Cu, Zn, Sn, and S), (ii) a mixture of the respective metal sulfides (CuS, ZnS, and SnS), and sulfur (S). They were made in each system in the form of both the raw powder of non-semiconducting cubic zincblende-type prekesterite and, after thermal treatment at 500 °C, of semiconductor tetragonal kesterite. Upon characterization, the nanopowders were subjected to high-pressure (7.7 GPa) and high-temperature (500 °C) sintering that afforded mechanically stable black pellets. Both the nanopowders and pellets were extensively characterized, employing such determinations as powder XRD, UV-Vis/FT-IR/Raman spectroscopies, solid-state Cu/Sn NMR, TGA/DTA/MS, directly analyzed oxygen (O) and hydrogen (H) contents, BET specific surface area, helium density, and Vicker's hardness (when applicable). The major findings are the unexpectedly high oxygen contents in the starting nanopowders, which are further revealed in the sintered pellets as crystalline SnO. Additionally, the pressure-temperature-time conditions of the HP-HT sintering of the nanopowders are shown (in the relevant cases) to result in the conversion of the tetragonal kesterite into cubic zincblende polytype upon decompression.
我们探讨了纳米粉末中以及高压高温烧结的半导体 kesterite CuZnSnS 纳米陶瓷中偶然氧存在的重要方面。最初的纳米粉末是通过机械化学合成路线从两个前驱体系统制备的,即(i)组成元素(Cu、Zn、Sn 和 S)的混合物,(ii)各自金属硫化物(CuS、ZnS 和 SnS)和硫(S)的混合物。在每个系统中,它们都以非半导体立方闪锌矿型 pre-kesterite 的原始粉末的形式以及在 500°C 下热处理后以半导体四方 kesterite 的形式存在。在表征过程中,纳米粉末经历了高压(7.7 GPa)和高温(500°C)烧结,得到了机械稳定的黑色颗粒。纳米粉末和颗粒都经过了广泛的表征,采用粉末 XRD、UV-Vis/FT-IR/Raman 光谱、固态 Cu/Sn NMR、TGA/DTA/MS、直接分析氧(O)和氢(H)含量、BET 比表面积、氦密度和维氏硬度(在适用的情况下)等测定方法。主要发现是起始纳米粉末中出人意料的高氧含量,在烧结颗粒中进一步揭示为结晶 SnO。此外,还展示了纳米粉末的高压高温烧结的压力-温度-时间条件,在相关情况下,导致在减压时四方 kesterite 转化为立方闪锌矿多型。