研究生: |
王信翔 Sin-Siang Wang |
---|---|
論文名稱: |
磁控濺鍍備製CIGS太陽能電池吸收層與TiO2薄膜之研究 The study on the CIGS solar cell absorber layer and TiO2 thin films by magnetron sputtering |
指導教授: |
修芳仲
Fang-jung Shiou |
口試委員: |
周振嘉
Chen-chia Chou 周賢鎧 Shyan-kay Jou 許春耀 Chun-yao Hsu 郭金國 Chin-guo Kuo 蔡豐羽 Feng-yu Tsai |
學位類別: |
博士 Doctor |
系所名稱: |
工程學院 - 機械工程系 Department of Mechanical Engineering |
論文出版年: | 2014 |
畢業學年度: | 102 |
語文別: | 中文 |
論文頁數: | 143 |
中文關鍵詞: | 銅銦鎵硒(CIGS)太陽能電池 、四元合金靶材 、前驅層 、快速熱處理製程 、硒化反應 |
外文關鍵詞: | quaternary-alloy target, rapid thermal process, precursor, selenized |
相關次數: | 點閱:463 下載:8 |
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本文研究利用非平衡磁控濺鍍(Unbalance magnetron sputtering)沉積銅銦鎵硒(CIGS)太陽能電池及TiO2薄膜。於不同直流功率及不同製程壓力沉積Mo背電極,顯示高直流功率(470 W)和低製程壓力(1 mtorr)條件下,可獲得較佳的Mo薄膜電阻率(1.3×10-5 Ω-cm)及反射率(62 %)。本研究以兩種不同方式製備CIGS太陽能電池吸收層,方式1: 使用CIGS四元合金(Cu:In:Ga:Se=25:17.5:7.5:50 at%)靶材,以射頻濺鍍沉積CIGS太陽能電池吸收層,結果顯示在較低的射頻功率(30 W)及製程壓力(2.5 mtorr)下,CIGS薄膜擁有最佳的元素比例(Cu:In:Se= 1:1:1.6)。方式2: 分別使用Cu0.75Ga0.25靶及In靶,直流濺鍍沉積CuGa (300 nm),改變不同In薄膜沉積時間,獲得適當Cu/(In+Ga)比例分別為0.80、1.00、1.20的前驅層,再經由快速熱處理製程(Rapid thermal processing, RTP),進行硒化反應成為CIGS吸收層。將TiO2薄膜於真空環境中進行退火(200~450 °C),顯示隨著退火溫度的增加,TiO2薄膜結構由非晶轉變為多晶結構,在紅外線波長到可見光範圍內,薄膜光穿透率也隨著退火溫度的提升獲得良好的改善。最後組合Mo、CIGS、In2S3、ZnO、GZO、TiO2及Al薄膜形成完整太陽能電池,量測其I-V曲線,顯示以方式1製備的CIGS吸收層經退火300 °C後,可穫得光電轉換效率(η)= 3.4%;以方式2(Cu/(In+Ga) 比例為1.00) 製備的CIGS吸收層經退火300 °C後,可穫得光電轉換效率(η)= 6.24%。
CuInGaSe2 solar cell and TiO2 thin film were grown onto soda-lime glass substrates by unbalance magnetron sputtering. The Mo thin film back contact layer used different direct current (D.C.) power and process pressure. By applying higher D.C. power (470 W) and lower process pressure (1 mtorr), findings show that the electrical resistivity of Mo films was 1.3 × 10-5 Ω-cm and the reflectivity was approximately 62%. In this study, the two different manufacturing processes were compared following the same absorber layer. The absorber layer of CIGS thin film were deposited by radio frequency (R.F.) magnetron sputtering, using the CIGS quaternary-alloy target (Cu:In:Ga:Se=25:17.5:7.5:50 at%). The results indicated that the best element ratio of CIGS thin film (Cu:In:Se= 1:1:1.6) could be achieved under lower R.F. power (30 W) and process pressure (2.5 mtorr). Another process, using D.C. magnetron sputtering of Cu0.75Ga0.25 alloy and In elemental targets, using a rapid thermal process of stacked elemental layers. The bottom layer of a 300 nm thick CuGa film was deposited. Thickness of the In layer was adjusted by adjusting the deposition time, to produce precursors with Cu/(In +Ga) atomic ratios of 0.80, 1.00, and 1.20. The optimized precursor was selenized under various temperatures, and the performance of the fabricated CIGS solar cells was analyzed.
TiO2 thin films annealed under different temperature (200~450 °C). The result showed that the TiO2 structure was changed from amorphous to polycrystalline when increase the annealing temperature. The TiO2 films optical transmittance was improved after annealed.
The structures of the CIGS thin film solar cell were Glass/Mo/CIGS/In2S3/ZnO/GZO/TiO2/Al. The experimental results showed that the absorber layer by CIGS quaternary-alloy targets, revealed a conversion efficiency of 3.4%. On the other hand, the absorber layer by means of both Cu0.75Ga0.25 alloy and In targets with stacked elemental layers. The stoichiometry of the metallic precursor was optimized, showed a conversion efficiency of 6.24% for the CIGS thin film solar cells.
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