Uneven crystallization of lead halide perovskite in the carbon-electrode based, low-temperature mesoscopic perovskite solar cells

Author:

Rong Qing1,Guo De’en1,Ma Jiao1,Lin Siyuan1,Huang Han1ORCID,Kong Deming1,Gao Yongli2ORCID,Zhou Conghua1ORCID

Affiliation:

1. Hunan Key Laboratory of Super-microstructure and Ultrafast Process, Hunan Key Laboratory of Nanophotonics and Devices, Institute of Super-microstructure and Ultrafast Process in Advanced Materials (ISUPAM), School of Physics and Electronics, Central South University, Changsha, Hunan 410083, People's Republic of China

2. Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA

Abstract

Crystallization of perovskite is monitored in carbon-electrode based, low-temperature, mesoscopic perovskite solar cells. Crystallographic and morphological properties of the perovskite are examined through changes in the film thickness of carbon-electrode or the volume of perovskite precursor. It is observed that, when a relatively thin carbon-electrode or large volume of perovskite precursor is used, perovskite crystallites mainly form on the device surface, leaving the bottom part of the device un-wetted. However, if a thicker carbon-electrode or less perovskite precursor is used, crystallization could be seen in the whole porous skeleton, and relative uniform distribution of perovskite crystallites is achieved. As such, uneven crystallization is observed. Such behavior is due to solvent evaporation on the surface, which facilitates nucleation processes on the surface, while retards crystallization on the bottom due to the Ostwald ripening effect. Charge transfer/recombination processes and photo-to-electric power conversion properties are studied. As expected, uneven crystallization results in retarded charge transfer and increased risk of recombination, and poor power conversion efficiency, for example, ∼3%. In contrast, uniform crystallization accelerates charge transfer and reduces recombination risk, and increases the efficiency to higher than 11% (AM1.5G, 100 mW/cm2).

Funder

National Science Fund for Distinguished Young Scholars

Natural Science Foundation of Hunan Province

National Science Foundation

Fundamental Research Funds for Central Universities of the Central South University

Innovation-Driven Project of Central South University

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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