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Synthesis and characterization of kesterite Cu2ZnSnTe4 via ball-milling of elemental powder precursors

机译:球磨元素粉前驱体合成钾钛矿Cu2ZnSnTe4及其表征

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A homologous series of kesterite light absorber materials Cu2ZnSnX4 (CZTX; X: S, Se, Te) can be used for realization of multi-junction solar cells. A stable member of the series (i.e. Cu2ZnSnTe4 (CZTTe)) was synthesized using a mechano-chemical route from its elemental precursors. Detailed characterization of the as synthesized as well as annealed CZTTe samples are being reported. XRD, Raman, TEM and SEM-EDS studies as well as Raman spectra confirm the formation of single-phase, stoichiometric, kesterite CZTTe nano-crystalline powder. The bandgaps of various samples of CZTTe were found in the range of 0.84-0.88 eV as confirmed by UV-Vis-NIR spectroscopy. The low band gap < 1 eV, coupled with the high absorption coefficient of similar to 10(4) cm(-1) suggests the possible use of this material as the absorber layer in the bottom cell of all kesterite multi-junction solar cells.
机译:一系列相同的钾盐沸石吸光材料Cu 2 ZnSnX 4(CZTX; X:S,Se,Te)可用于实现多结太阳能电池。使用机械化学方法从其元素前体合成了该系列的稳定成员(即Cu2ZnSnTe4(CZTTe))。据报道,合成的和退火的CZTTe样品的详细表征。 XRD,拉曼,TEM和SEM-EDS研究以及拉曼光谱证实了单相,化学计量的,钾钛矿型CZTTe纳米晶体粉末的形成。通过UV-Vis-NIR光谱证实,发现各种CZTTe样品的带隙在0.84-0.88 eV的范围内。小于1 eV的低带隙,再加上类似于10(4)cm(-1)的高吸收系数,表明该材料有可能用作所有Kesterite多结太阳能电池底部电池的吸收层。

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