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April 18, 2026ACS Energy Letters0 citations

Dose-Dependent Transition in Wide-Bandgap Tin-Based Perovskite Solar Cells under Low-Dose γ-Irradiation

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SCSungWon ChoWCWon S. ChoiDLDa Seul Lee

Key Points

  • This research aims to understand how tin-based perovskite solar cells respond to low-dose γ-irradiation and the associated defect evolution.
  • Examined γ-irradiation effects on wide-bandgap tin-based perovskite solar cells
  • Analyzed cumulative doses from 0 to 500 Gy
  • Assessed changes in device efficiency and defect states
  • Low doses (≤100 Gy) improved device efficiency from 6.16% to 6.79%
  • Higher doses (≥100 Gy) caused irreversible performance degradation due to Sn2+ oxidation
  • Defined a dose-dependent transition in defect dynamics within the 10–100 Gy interval

Abstract

Wide-bandgap (WBG) tin-based (Sn-) perovskites possess redox-active Sn2+/Sn4+ chemistry that fundamentally alters defect evolution under ionizing environments; however, their cumulative total ionizing dose (TID) response remains poorly understood. Here, we investigate the γ-irradiation response of WBG Sn-perovskite solar cells (PSCs) over cumulative doses from 0 to 500 Gy to elucidate cumulative TID-driven defect evolution. Low-dose exposure (≤100 Gy) reduces nonradiative recombination losses through radiation-assisted reconfiguration of pre-existing shallow defect states, increasing the average device efficiency from 6.16% to 6.79%. In contrast, higher doses (≥100 Gy) induce progressive Sn2+ oxidation, halide depletion, and deep-level trap formation, resulting in irreversible performance degradation. By delineating a transition from a low-dose defect-reconfiguration regime to a high-dose degradation regime, this work establishes an observed dose-dependent transition within the 10–100 Gy interval under the present sampling resolution and defines a redox-defect-coupled framework for understanding radiation-driven defect evolution in Sn-perovskites.

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Cite This Study

Cho et al. (2026) studied this question.

synapsesocial.com/papers/69e31ec840886becb653e7edhttps://doi.org/10.1021/acsenergylett.6c00190
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