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Synchronized B-site alloying for high-efficiency inorganic tin-lead perovskite solar cells

  • Ting Zhang
  • , Feng Wang
  • , Hao Chen
  • , Feng Qian
  • , Jian Li
  • , Hualin Zheng
  • , Shihao Yuan
  • , Xuefeng Peng
  • , Yafei Wang
  • , Jiang Huang
  • , Hao Cui
  • , Zhinong Yu
  • , Zhi David Chen
  • , Shibin Li

Producción científica: Articlerevisión exhaustiva

34 Citas (Scopus)

Resumen

Inorganic tin-lead perovskites with low bandgap (1.2-1.4 eV) are desired absorber materials for solar cells owing to their ideal bandgap and compositional stability. However, such tin-lead perovskites are currently subject to inferior power conversion efficiency (PCE) and the origin remains unclear. Here, for the first time, we report the metal-cation-derived unsynchronized crystallization behavior of inorganic tin-lead perovskite, exemplifying by a representative composition CsPb0.7Sn0.3I3. A tin-perovskite-targeted crystallization modulation agent, 1-(4-fluorophenyl) piperazine (1-4FP), is introduced to synchronize the B-site alloying through its strong targeted bonding with SnI2, resulting in substantially enhanced film quality with better morphology and photoelectrical properties. Furthermore, first-principles molecular dynamics simulations reveal that the agent regulates the crystallization route toward the pure phase of CsPb0.7Sn0.3I3 by suppressing the preforming of tin perovskite. With our proposed approach, the best device attains PCE of 17.55%, which is record-high for inorganic tin-lead perovskite solar cells. In addition, treated devices show excellent stability with only 10% and negligible loss after being exposed to 1 sun intensity for 700 h and being stored in N2 after over 4000 h, respectively. Our findings open a new avenue of crystallization route design in inorganic tin-lead perovskites, so as to obtaining high-quality perovskite films and associated solar cells.

Idioma originalEnglish
Número de artículo041417
PublicaciónApplied Physics Reviews
Volumen10
N.º4
DOI
EstadoPublished - dic 1 2023

Nota bibliográfica

Publisher Copyright:
© 2023 Author(s).

Financiación

This work was supported by the National Natural Science Foundation of China (62104028 and 62174021), Creative Research Groups of the National Natural Science Foundation of Sichuan Province (2023NSFSC1973), the Natural Science Foundation of Sichuan Province (2022NSFSC0899), and China Postdoctoral Science Foundation (2021M700689). This work was also sponsored by the Sichuan Province Key Laboratory of Display Science and Technology.

FinanciadoresNúmero del financiador
Sichuan Province Key Laboratory of Display Science and Technology
National Natural Science Foundation of China (NSFC)62104028, 62174021
National Natural Science Foundation of China (NSFC)
China Postdoctoral Science Foundation2021M700689
China Postdoctoral Science Foundation
Natural Science Foundation of Sichuan Province2022NSFSC0899, 2023NSFSC1973
Natural Science Foundation of Sichuan Province

    ASJC Scopus subject areas

    • General Physics and Astronomy

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