Effects of Pressure on Optoelectronic Properties of Perovskite Thin Films Fabricated via Radio Frequency Sputtering

  • Sittan Wongcharoen
  • , Ratchatee Techapiesancharoenkij
  • , Itaru Raifuku
  • , Tomoya Goda
  • , Krittin Auewattanapun
  • , Hidenori Kawanishi
  • , Yvan Bonnassieux
  • , Pere Roca i Cabarrocas
  • , Kosuke Hara
  • , Yukiharu Uraoka

Research output: Contribution to journalArticlepeer-review

Abstract

Perovskite thin films were fabricated via the radio frequency (RF) sputtering process, which could provide great control over the crystal structure and uniformity of the films. Lead sulfide was chosen as a precursor for the lead source and further converted to lead iodide (RF-PbI2) and methylammonium lead iodide (RF-CH3NH3PbI3: RF-MAPbI3) through a two-step gas-phase reaction. The sputtering pressure was varied from 0.3 to 0.9 Pa to investigate its influence on the characteristics of the RF-PbI2 and RF-MAPbI3 films. The increase in the pressure transformed the structure of the RF-PbI2 films from a dense to porous structure; meanwhile, the grain growth behavior of the RF-MAPbI3 was also observed after the conversion. Grain growth reduced the grain boundary density and decreased carrier trapping. This reduction of grain boundaries also enhanced light scattering and improved the light-harvesting properties of the films, as confirmed by a higher absorption coefficient in the visible region. The decrease in the grain boundaries also reduced the recombination centers and improved the carrier lifetime. Nevertheless, RF-MAPbI3 thin films fabricated with pressures exceeding 0.5 Pa presented a highly porous structure and poor crystallinity. Thus, these findings indicated an optimal pressure of 0.5 Pa for the RF-sputtered lead sulfide (RF-PbS) precursor that resulted in an optimal perovskite thin film prepared via this commercial method, indicating a promising pathway toward robust, controllable, and scalable perovskite optoelectronic devices.

Original languageEnglish
Pages (from-to)61627-61637
Number of pages11
JournalACS Omega
Volume10
Issue number50
DOIs
Publication statusPublished - 23 Dec 2025

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