2021
DOI: 10.1016/j.bsecv.2020.05.004
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Investigation of absorber and heterojunction in the pure sulphide kesterite

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Cited by 7 publications
(3 citation statements)
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“…Figure 3a shows the Raman spectra of the CZTS sample. The appearance of the high-intensity peaks at about 288 cm À1 and 337.5 cm À1 corresponds to the two A modes of the kesterite structure whereas the less intense peaks at 366.3 cm À1 and 373 cm À1 correspond to the E(LO) and B(LO) modes [29][30][31][32]. Figure 3b shows the Raman spectra of the CCZTS sample.…”
Section: Morphological and Structural Characterizationmentioning
confidence: 99%
“…Figure 3a shows the Raman spectra of the CZTS sample. The appearance of the high-intensity peaks at about 288 cm À1 and 337.5 cm À1 corresponds to the two A modes of the kesterite structure whereas the less intense peaks at 366.3 cm À1 and 373 cm À1 correspond to the E(LO) and B(LO) modes [29][30][31][32]. Figure 3b shows the Raman spectra of the CCZTS sample.…”
Section: Morphological and Structural Characterizationmentioning
confidence: 99%
“…The preparation work-up and, specifically, the drying stage in air in the “wet” mechanochemical synthesis method, constitutes yet another oxygen source, possibly even more acute, since one deals at this stage with very reactive, high-surface-area nanopowders exposed to air for relatively long and variable periods of time. As a result, such oxidation by-products are detected for kesterite samples as metal sulfates including copper sulfate pentahydrate CuSO 2 •5H 2 O, zinc sulfate monohydrate ZnSO 4 •H 2 O, and, possibly, hydrated tin oxide SnO 2 •xH 2 O not only in the mechanochemical synthesis method [ 4 , 5 , 9 ] but also in other preparation routes [ 10 , 11 , 12 ]. It is instructive to note that in some kesterite studies, the presence of oxygen-bearing species is evident from inspection of the data, although it is not specifically acknowledged or appropriately commented on by authors [ 13 ] (e.g., XPS survey scans with the apparent O 1s band in the range of 529–531 eV for oxides or the S2p 3/2 /S2p 1/2 bands in the range of 167–172 eV for the sulfate group [SO 4 ] −2 ).…”
Section: Introductionmentioning
confidence: 99%
“…Thin films of CZTS are composed of abundant materials on earth with low toxicity (Copper (Cu), Zinc (Zn), Tin (Sn) and Sulfur (S)), and they have p-type conductivity, large band gap (in the range of 1.4-1.6 eV) with a high absorption coefficient (over 10 4 cm -1 ) that make it an excellent and promising material for solar cells [6]. CZTS thin films can be prepared by various physicochemical methods such as pulsed laser deposition [7], electrochemical deposition [8], chemical bath deposition [9], spray pyrolysis [10] and spin coating [11], etc. However, some of these methods suffer from expensive hardware requirements and significant power consumption.…”
Section: Introductionmentioning
confidence: 99%