Applied Science and Convergence Technology 2024; 33(6): 156-159
Published online November 30, 2024
https://doi.org/10.5757/ASCT.2024.33.6.156
Copyright © The Korean Vacuum Society.
Muntae Hwang , Il-Wook Cho , Jaewon Oh , Hyunbok Lee , and Mee-Yi Ryu ∗
Department of Physics and Institute of Quantum Convergence Technology, Kangwon National University, Chuncheon 24341, Republic of Korea
Correspondence to:myryu@kangwon.ac.kr
This is an Open Access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (https://creativecommons.org/licenses/by-nc-nd/4.0/) which permits non-commercial use, distribution and reproduction in any medium without alteration, provided that the original work is properly cited.
Using a Lewis base additive is essential for synthesizing uniform perovskite because it forms an intermediate phase during the perovskite solution process which slows the crystallization rate. Synthesizing CsFAPbI3 with a high concentration of cesium in an ambient environment, using dimethyl sulfoxide (DMSO) as a Lewis base additive, leads to the formation of δ-CsPbI3, which reduces light absorption in the perovskite. To suppress δ-CsPbI3 formation, this study utilizes N-methyl-2-pyrrolidone (NMP) as the Lewis base additive. The perovskite synthesized with NMP effectively suppresses δ-CsPbI3. However, there is no significant difference in solar cell performance compared to those synthesized with DMSO. This lack of improvement can be attributed to the incompatible interaction between ethyl acetate and NMP, which increases non-radiative recombination and reduces carrier lifetime.
Keywords: Perovskite, Cesium, Solar cell, Dimethyl sulfoxide, N-methyl-2-pyrrolidone