Approaches for thermodynamically stabilized CsPbI3 solar cells

被引:110
作者
Li, Zhizai [1 ]
Zhou, Faguang [1 ]
Wang, Qian [1 ]
Ding, Liming [2 ]
Jin, Zhiwen [1 ]
机构
[1] Lanzhou Univ, Sch Phys Sci & Technol, Key Lab Magnetism & Magnet Mat MoE, Key Lab Special Funct Mat & Struct Design,MoE,Nat, Lanzhou 730000, Peoples R China
[2] Natl Ctr Nanosci & Technol, Ctr Excellence Nanosci CAS, Key Lab Nanosyst & Hierarch Fabricat CAS, Beijing 100190, Peoples R China
基金
中国国家自然科学基金;
关键词
CsPbI3; Perovskite; Solar cells; Thermodynamically; Stability; CESIUM LEAD IODIDE; HALIDE PEROVSKITES; ALPHA-CSPBI3; PEROVSKITE; HIGHLY EFFICIENT; QUANTUM DOTS; STABLE CSPBI3; THIN-FILMS; PHASE; PERFORMANCE; CSPBL(3);
D O I
10.1016/j.nanoen.2020.104634
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
With its suitable bandgap (<1.73 eV), excellent optoelectronic properties and ideal thermo-stability, cesium lead halide, CsPbI3, is a promising candidate for next-generation photovoltaics (PVs). However, its instable structure (perovskite black phase can transform to non-perovskite yellow phase at room temperature) limits further development. Since the first report in 2014, much efforts have been made to stabilize the structure (black phase), and the corresponding inorganic perovskite solar cells (PSCs) have made great progress in terms of power conversion efficiency (PCE) which increased from 0.09% to 19.03%. In this review, we summarize the intrinsical instability of CsPbI3, and discuss the recent works in improving the stability of CsPbI3 from four aspects: (1) ionic incorporation; (2) metastable phases; (3) reduced dimensions; (4) steric hindrance. Finally, the problems that still exist and the possible directions for solving them are presented.
引用
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页数:14
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