Earth abundant, non-toxic, and cost-effective CZTS absorber material has been attracted much attention for thin film solar cells. Rapid development in achieving the high efficiency in CZTS-based solar cells is hindered by the narrow phase stability of...
Earth abundant, non-toxic, and cost-effective CZTS absorber material has been attracted much attention for thin film solar cells. Rapid development in achieving the high efficiency in CZTS-based solar cells is hindered by the narrow phase stability of the quaternary phase, Cu2ZnSnS4, and the existence of other complex secondary phases and defects. TEM is a powerful technique to provide information on the microstructure and chemistry of defects, interfaces, and junctions in polycrystalline thin-film solar cells. This information can provide crucial insights for understanding the performance of thin film solar cells. In this thesis, microstructural characterization of the CZTS absorbers by sputtering method for the wide production of kesterites solar cells have been studied using TEM.
First, the temperature dependent phase evolution of CZTS films is systematically studied the stacked ZnS/SnS2/Cu films sulfurized at different temperatures. Based on the experimental evidence the plausible phase evolution mechanism is proposed.
Second, The phase evolution process in sulfurized CZTS thin films prepared using different sulfurization times was described through ex-situ analysis, and a mechanism for Cu-S and Zn-S based secondary phase segregation was proposed. In addition to performing conventional XRD and RAMAN characterization, a sulfurization temperature-dependent phase evolution mechanism was proposed. The formation of secondary phases (Cu2S and ZnS) in CZTS films with longer annealing times was shown by TEM and STEM-mapping analyses. The driving force for Cu-S and Zn-S based secondary phase segregation was the favored Sn (II) oxidation state at high and long sulfurization temperatures.
Third, the phase evolution pathways have proposed for kesterite CZTS and CZTSe thin films by annealing of sputtered metallic precursor under chalcogenide atmospheres through experimental observation during the annealing process. Unlike phase evolution pathway for kesterite CZTS thin film by annealing of S-contained precursor, the Cu2-xS secondary phase was observed in the thin films sulfurized at temperature of 450 °C, even though no observation of this phase was made using XRD patterns and Raman spectra. Conversely, the Cu2SnSe3 phase was not observed during selenization process. The binary phases including Cu2-xSe, ZnSe, and SnSe2 were directly transformed to the kesterite CZTSe phase and they became large with micronsized grains. This study suggests variable and useful information for the preparation of kesterite CZTS and CZTSe thin films that can be used as high quality absorber materials in the high efficiency and low cost TFSC devices.
Finally, the CZTS-based thin film solar cells were fabricated Al/AZO/i-ZnO/CdS/CZTS-Se/Mo/Glass multi-structure and recorded a cell efficiency 2.10 % for CZTS TFSC and 2.44 % for CZTSe TFSC, respectively.