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作者(中文):陳奕如
作者(外文):Chen, Yi-Ju
論文名稱(中文):利用金奈米粒子之表面電漿效應提升非真空製程銅銦鎵硒太陽能電池之吸光特性及元件表現
論文名稱(外文):Enhancement of Light Absorption by Plasmonic Nanoparticles For Non-Vacuum Cu(In,Ga)Se2/CuInSe2 Solar Cell
指導教授(中文):闕郁倫
指導教授(外文):Chueh, Yu-Lun
口試委員(中文):沈昌宏
王祥辰
口試委員(外文):Chang-Hong Shen
Hsiang-Chen Wang
學位類別:碩士
校院名稱:國立清華大學
系所名稱:材料科學工程學系
學號:101031608
出版年(民國):103
畢業學年度:102
語文別:英文
論文頁數:61
中文關鍵詞:銅銦鎵硒太陽能電池表面電漿效應金奈米粒子
外文關鍵詞:plasmonicCIGS solar rcellAu nanoparticles
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銅銦鎵硒(CIGS)為一種直接能隙材料,吸光範圍寬,做成太陽能電池具高光電轉換效率,目前世界紀錄為20.8%。CIGS太陽能電池材料中的銦、鎵、硒元素地球上含量稀少總量有限,故如何減少吸收層材料使用並保持高效率為目前研究重點之一。金屬粒子具表面電漿效應。當金屬粒子受光照產生表面電漿共振時,其對光散射及吸收的截面積均會增加。若將此粒子置於太陽能電池吸收層中可增加光被利用的機率,使元件整體表現提升。本研究利用金奈米粒子的表面電漿效應提高CIGS元件整體表現。並以薄膜光學性質的量測及模擬解釋表面電漿效應對元件的增益機制。因為金奈米粒子的散射及吸收效應使光被CIGS薄膜的利用率提高,加入金奈米粒子的元件其光電流及光電轉換效率均有顯著提升。如此作法可成功減少吸收層材料使用並有機會於未來做出高效率超薄型可撓式CIGS薄膜太陽能電池。
In this work, we successfully demonstrated plasmonic Cu(InGa)Se2-based thin film solar cell prepared by a non-vacuum process. Cu(In,Ga)Se2, (CIGS) is a direct band gap semiconductor material that can be used as the absorption layer in thin film solar cell with the highest efficiency of 20.8 % so far. In recent years, researchers have made a lot of efforts on reducing the usage of materials in order to reduce material cost. Many possible approaches have been adopted to light absorption management to maintain cell efficiency while reducing the thickness of these absorption layers, such as nanostructured surface. Plasmonic effect, which is one of approaches for light trapping, has been successfully applied on polymer tandem solar cell and Si solar.
In the first study, Au nanoparticles (Au NPs) were introduced into CIGS/CdS and CdS/iZnO of CIGS device, respectively. Based on angle-dependent reflectance measurement, an enhanced light absorption in the range of 400~600 nm can be observed, which is consistent with the increasing external quantum efficiencies (EQE) of these devices. 8.52% enhancement of short circuit current (Jsc) and 24.7% improvement of power conversion efficiency have been attained by the light trapping effect utilizing plasmonic effect.
However, it remains challenges for applying Au NPs into Cu(InGa)Se2-based solar cells because Au NPs will react with In and Cu during high temperature annealing processes. In order to address this issue, development of thermal-stable protection shell was developed in the second study of the thesis. In brief, Au@SiO2 NPs were mixed with CuInS2 nanocrystal ink homogenously and experienced at high temperature selenization process to form CISe2 thin film layer where the plasmonic CuInSe2 (CISe2) solar cell with enhanced conversion efficiency by employing Au-SiO2 core-shell nanoparticles (Au@SiO2 NPs) can be achieved. SEM images reveal that the SiO2 shell can protect Au NPs intact after the high temperature annealing process. Consequently, under AM1.5G irradiation, the short circuit current (Jsc), open circuit voltage (Voc) and power conversion efficiency (η) have been improved by 13 %, 5 % and 17 % in average, respectively. This work successfully demonstrated enhanced light absorption scheme utilizing the Au and Au@SiO2 NPs within chalcopyrite solar cells and may have beneficial potential to other thin film photovoltaic devices systems.


Table of Content
Abstract i
Acknowledgement iii
Table of Content iv
List of Figures vi
List of Tables ix
Acronyms x
Chapter1 Introduction 1
1.1 Preface 1
1.2 CuInxGa(1-x)Se2 (CIGS) solar cell 3
1.3 Plasmonics Effect 7
1.4 Plasmonic enhanced photovoltaic 10
Chapter2 Experimental Sections 11
2.1 Experimental Sections 11
2.1.1 Particles synthesis 11
2.1.2 Device fabrication process 12
2.2 Instruments 15
Chapter3 Toward Omnidirectional Light Absorption by Plasmonic Nnaoparticles For High Efficiency Flexible Non-Vacuum Cu(In,Ga)Se2 Thin Film Solar Cell 23
3.1 Experimental Design and process 23
3.2 Results and Discussions 24
3.3 Summary 42
Chapter4 Plasmon-Enhanced Light Absorption Of Non-Vacuum CuInSe2 Thin Film Solar Cell by Absorber Layer-Incorporated Au-SiO2 core-shell Nanoparticles 43
4.1 Experimental Design 43
4.2 Results and Discussion 45
4.3 Summary 56
Chapter5 Conclusions 57
Reference 59




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