研究目的
Investigating the microstructure of chalcopyrite-type CuInSe2 and kesterite-type Cu2ZnSnSe4 absorber layers in thin film solar cells to understand their impact on solar energy conversion efficiency.
研究成果
The microstructure analysis of chalcopyrite-type and kesterite-type absorber layers in thin film solar cells provides valuable insights into the impact of process parameters, such as temperature and sodium incorporation, on the structural and electronic properties of the absorbers. The studies demonstrate that higher process temperatures and the presence of sodium can significantly influence microstrain and lattice parameters, which in turn affect the solar cell performance. The findings contribute to a better understanding of the factors that determine the efficiency of thin film solar cells and highlight the importance of microstructure analysis in the development of high-performance photovoltaic devices.
研究不足
The resolution of conventional X-ray diffractometers limits the detectable domain sizes to around 100 nm and below, making it difficult to assess the impact of sodium on domain size in some samples. Additionally, the separation of size and strain effects can be challenging, and the comparability of microstructure information obtained by different setups may be restricted to qualitative evaluations.