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Non-toxic FASnI3 perovskite on nanostructured black silicon for light-trapping-enhanced infrared photodetectionopen access

Authors
Jung, JaehoonSun, KyoungjunSo, YuhanSung, JunyeongYoun, Yeo BinKim, Nu RiYoon, Se WonBaek, Jae WooLee, HyeonryulKim, HyeonghunLee, Jong-HoonKwon, SooncheolKim, Min-Woo
Issue Date
May-2026
Publisher
한국물리학회
Keywords
Black silicon (b-Si); FASnI3 (formamidinium tin tri-iodide); Infrared (IR) photodetectors; Lead-free perovskites; Nanostructured substrates; Solution-processed optoelectronics
Citation
Current Applied Physics, v.85, pp 147 - 156
Pages
10
Indexed
SCIE
SCOPUS
KCI
Journal Title
Current Applied Physics
Volume
85
Start Page
147
End Page
156
URI
https://scholarworks.dongguk.edu/handle/sw.dongguk/63888
DOI
10.1016/j.cap.2026.01.012
ISSN
1567-1739
1878-1675
Abstract
Lead(Pb)-based perovskites have exhibited exceptional light absorption characteristics and superior photoconversion efficiencies in optoelectronic applications but face commercialization limits due to Pb toxicity and chemical instability. Tin(Sn)-based perovskites, particularly formamidinium tin triiodide (FASnI<inf>3</inf>), have emerged as promising non-toxic alternatives for infrared (IR) photodetection. Here, we fabricate FASnI<inf>3</inf> thin films on nanostructured black silicon (b-Si) substrates and compare with films on flat silicon (f-Si) substrates to systematically evaluate their IR photodetector performance, including responsivity, detectivity, and external quantum efficiency (EQE). The b-Si based devices yield a response speed approximately 20 times faster than that of f-Si, driven by enhanced light trapping at the nanostructured surface that boosts photon absorption and carrier generation, alongside 2 times higher detectivity depending on incident optical power. Time-dependent PL results suggest a modest substrate-enabled mitigation of ambient degradation trends. These substrate-dependent improvements in performance highlight b-Si as a viable platform for realizing non-toxic perovskite IR photodetectors. © 2026 Korean Physical Society
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