IMR OpenIR
a-Si薄膜的激光表面晶化行为研究
其他题名Surface Crystallization Behavior of a-Si Thin Films Induced by Lasers
崔连武
学位类型硕士
导师闻立时
2009-05-20
学位授予单位中国科学院金属研究所
学位授予地点金属研究所
学位专业材料加工工程
关键词A-si薄膜 准分子激光 表面晶化 数值模拟 温度场
摘要作为目前最具有发展前景的硅基薄膜太阳电池,具有原材料取之不尽、绿色环保以及成本低廉等优点,因此得到广泛的研究与应用。然而光电转换效率较低、稳定性不好一直是制约硅基薄膜电池发展的瓶颈。本论文主要利用激光表面晶化的方法,在a-Si薄膜表面上制备一层μc-Si层,并以此作为薄膜电池的本征吸收层,进而达到提高电池转换效率和稳定性的目的。晶化层的微观结构对性能起决定性作用,因此,本文通过研究不同准分子激光对a-Si薄膜的表面晶化行为,并对温度场进行数值模拟,从而建立激光工艺参数与晶化层微观结构的关系,为激光表面晶化法制备μc-Si /a-Si复合薄膜提供实验依据。同时,也为研究制备稳定高效的第三代薄膜太阳电池打下理论基础。 本文分别研究了KrF和ArF准分子激光对a-Si薄膜的表面晶化行为,包括a-Si薄膜的表面晶化阈值、激光能量密度及照射脉冲数对薄膜结晶度的影响、晶化后的薄膜表面形貌及晶化层延深度的分布等。通过实验发现:a-Si薄膜的表面晶化阈值约为110mJ/cm2,并且不受照射脉冲数的影响;激光能量密度是影响薄膜结晶度的主要因素,随激光能量密度升高,薄膜表面结晶度增大;通过多脉冲照射也可以提高薄膜的结晶度,尤其在激光能量密度较低时,但随着激光能量密度升高,作用的效果变得不明显;晶化层的表面SEM和TEM表征结果显示,随着激光能量密度升高,薄膜表面结晶程度提高,晶化层中微晶晶粒尺寸变大,但当能量密度高于一定值时,晶粒均匀性变差,并且表面有大颗粒出现,薄膜质量变差;对ArF激光晶化的薄膜进行截面TEM表征发现,随激光能量密度升高,晶化层的深度加大,并且呈抛物线规律递增。对比研究表明,相同条件下,KrF准分子激光晶化时薄膜结晶度更高、晶化层深度更深;而采用ArF激光晶化时,微晶层的晶粒更加均匀,薄膜表面质量更好。因此,采用KrF准分子激光进行晶化时,较佳的激光能量密度范围是110~150mJ/cm2;而采用ArF准分子激光时,较佳的激光能量密度范围是120~180mJ/cm2。 通过建立数学模拟对激光晶化a-Si薄膜的温度场进行了数值模拟计算,主要研究了激光波长、能量密度和衬底温度等对薄膜温度场的影响。计算结果显示:随着激光波长和脉宽的增加,薄膜的表面熔化阈值增大,在脉宽一定时,采用波长为300~350nm之间的激光照射时薄膜表面熔化阈值最低;薄膜表面熔化时间、熔化层深度和表面最高温度都随激光能量密度的升高而增大,并且相同条件下,KrF (248nm) 激光比ArF (193nm) 激光的作用效果更加明显;衬底温度主要影响薄膜表层熔化的时间,即提高衬底温度可以显著的增加薄膜表面熔化时间,而对于薄膜熔化深度和表面温度的影响次之。通过将计算结果与本文及他人实验结果进行对比,验证了模型的准确性与适用性。
其他摘要Si-based Thin Film Solar Cells, as the most promising solar cells since now, have been studied intensively and applied to many areas,because of their advantages, such as the very abundant storage of Si in the earth, the environmental friendly characteristic, and the very low manufacturing cost. But the low efficiency and bad stability still confined their development. In this work, laser crystallization method was used to crystallize the surface layer of the a-Si thin films, and the resulting μc-Si/a-Si composite films were proposed to be as the intrinsic absorbing layer in thin film solar cells, so as to improve the efficiency and stability. Since the microstructure of the crystallized layer directly determines the performance of solar cells, in this work we tried to build up relationships between the microstructure of the crystallized layer and laser parameters by studying the crystallization behaviors of a-Si thin films induced by different excimer lasers as well as making numerical simulations of the temperature field within the films. The aim of this work is to try to provide experimental and theoretical basis for making μc-Si /a-Si composite films by laser surface crystallization method as well as making efforts for the development of the third generation of high-efficient and stable solar cells. In this work, the crystallization behaviors of a-Si thin films induced by KrF and ArF were studied, including the surface crystallization threshold of the as-deposit a-Si thin films, the influences of laser fluence and laser shots on films’ crystallinity, the surface morphology and crystallizing layers' distributions along depth, and so on. The results indicated that the laser surface crystallization threshold of the as-deposit a-Si thin films was near 110mJ/cm2, which was independent of shot numbers. The crystallinity could be increased mainly by increasing laser fluence, however the shot numbers also had an obvious effect on it when laser fluence was low. SEM and TEM view of the crystallizing layer showed that the crystallinity and mean grain size were both increased as laser fluence was increased; but when laser fluence was over a certain value, the uniformity of the grains lowered and some bigger grains showed up, leading to bad film qualities. TEM cross-section view of the ArF excimer laser crystallized thin films showed that the crystallized μc-Si layer was deepened by increasing laser fluence, and followed the parabola law. By comparing the experimental results we found that, under the same conditions, surface crystallization of KrF excimer laser resulted in higher crystallinity and deeper crystallized μc-Si layer, and ArF excimer laser resulted in more uniform grain sizes and higher surface quality. So it was better when laser fluence was 110~150 mJ/cm2 for KrF excimer laser crystallization, and 120~180mJ/cm2 for ArF excimer laser crystallization. Temperature field simulations were carried out by numerical method, focusing on the influences of laser wavelength, laser fluence and substrate temperature on the temperature field within the films. The simulation results showed that the surface melting threshold of a-Si thin films was increased as laser wavelength and pulse duration increased. And when pulse duration was constant, the lowest surface melting threshold was obtained at wavelength of 300~350nm. Surface melting duration, melting layer depth and surface highest temperature of the films were all increased as laser fluence was increased; and under the same conditions, the effects of KrF(248nm) laser were more obvious than that of ArF(193nm) laser. Substrate temperature mainly had an influence on surface melting duration of the films, that was to say, the surface melting duration time would increased quickly by increasing substrate temperature, and would have less effects on melting depth and surface temperature of the films. By comparing the simulation results with experimental results of this work and with other researching results, the accuracy and applicability of the numerical simulation were verified.
页数95
语种中文
文献类型学位论文
条目标识符http://ir.imr.ac.cn/handle/321006/17246
专题中国科学院金属研究所
推荐引用方式
GB/T 7714
崔连武. a-Si薄膜的激光表面晶化行为研究[D]. 金属研究所. 中国科学院金属研究所,2009.
条目包含的文件
条目无相关文件。
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[崔连武]的文章
百度学术
百度学术中相似的文章
[崔连武]的文章
必应学术
必应学术中相似的文章
[崔连武]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。