本實驗是研究銅鋅錫硒硫Cu2ZnSn(SSe)4薄膜在太陽能電池吸收層材料之特性。其製程是利用鋅與硒、錫與硒以1:1的比率配置以及添加少量的碘化鉀KI鹽類並在1050℃的溫度下於石英管中熔煉成二元化合物,然後添加1:1的硫化銅,利用濕式球磨法來製備混和物之漿料以形成貧銅(Cupper poor)、計量比(Stoichiometric)、富銅(Cupper rich)之五元化合物(分別為Cu/Zn+Sn原子百分比=0.8、1.0、1.2、1.5),並利用旋轉塗佈法將漿料塗佈於玻璃基板上以形成前驅層薄膜。接著,將樣品置於爐管內進行快速退火製成(RTA),溫度分別為300℃、400℃及500℃,退火時間為10分鐘。 利用感應耦合電漿質譜分析儀(ICP)和能量散色光譜儀(EDS)來測量薄膜之成分分析、掃描式電子顯微鏡(SEM)觀察薄膜的表面形貌與橫截面樣貌、X光繞射分析儀(XRD)判斷薄膜的晶體結構、紫外光可見光光譜儀分析薄膜之光學性質。由實驗結果得知Cu/Zn+Sn=1.5之Cu2ZnSn(SSe)4薄膜,在退火溫度為500℃下可以得到鋅黃錫礦結構,有較好的結晶性,其能隙值約在1.4eV~1.5eV之間。
The experiment is investigate on the application of characteristic Cu2ZnSn(SSe)4 for solar cell absorber layer materials. First of all, zinc, selenium and tin, selenium the configuration used in a proportion of one to one and add a small amount of potassium iodide. Were melted in quartz tubes at 1050 oC to form binary compound, then add 1: 1 copper sulfide. Inks of the pentanary compound were made using wet-type ball milling four ingots from Cu-poor, stoichiometric to Cu-rich mixtures (Cu/Zn+Sn atomic ratio = 0.8, 1.0, 1.2 and 1.5, respectively), and printed onto a glass substrate to form a precursor film by spin coating. Then, the samples were heated with rapid thermal annealing (RTA) in a furnaceat 300 oC, 400 oC, 500 oC, respectively, for 10 minutes. The compositions of the films were determined by inductively coupled plasma-mass spectrometer (ICP) and energy dispersive spectroscopy (EDS) measurements. Surface and cross-section morphologies were observed by scanning electron microscopy (SEM). The crystal structure of the films was analyzed by X-ray diffraction (XRD). Optical properties were recorded by UV-Vis-NIR spectrometer. Based on the results of the experiments, the thin films (Cu/Zn+Sn atomic ratio = 1.5) with Kesterite structure was obtained by annealing temperature of 500 oC. It also showed higher crystallinity, and the band gap was 1.4 eV~ 1.5 eV.