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    Enhancing band-edge nonradiative recombination lifetimes in I-II2-III-VI4 chalcogenides via orbital-phonon synergy

    Xinwei Guo, Wenhan Zhou*, Shengli Zhang†, and Haibo Zeng‡

    • MIIT Key Laboratory of Advanced Display Materials and Devices, Jiangsu Engineering Research Center for Quantum Dot Display, School of Materials Science and Engineering, Institute of Optoelectronics & Nanomaterials, Nanjing University of Science and Technology, Nanjing, Jiangsu 210094, China

    • *Contact author: zhouwenhan@njust.edu.cn
    • †Contact author: zhangslvip@njust.edu.cn
    • ‡Contact author: zeng.haibo@njust.edu.cn

    Phys. Rev. B 112, 165203 – Published 20 October, 2025

    DOI: https://doi.org/10.1103/b1mb-2yrj

    Abstract

    Balancing efficiency enhancement and cost reduction is crucial for advancing solar energy and photovoltaic devices. One of the primary sources of energy loss, leading to reduced efficiency, is nonradiative electron-hole recombination within these devices. In this study, we comprehensively investigated the nonradiative properties of excited-state carriers in quaternary Kesterite (KS) and Stannite (ST) phase I−II2−III−VI4 chalcogenide compounds using first-principles calculations combined with nonadiabatic molecular dynamics (NAMD). We identified the characteristics of chemical bond elongation, electron localization and bandgap fluctuations induced by cation modulation. Specifically, forming quaternary structures by introducing Zn and substituting In3+ with Ga3+ and Cu+ with Ag+ resulted in increased bandgaps. Through a detailed analysis of orbital and vibrational components, we elucidated the principles for regulating nonadiabatic coupling and carrier lifetimes, including strategies to suppress the t2 orbital of I-site cations, low-frequency optical phonons and anti-Zeno effects. Compared with the KS structure, the ST structure retains higher symmetry, with suppressed low-frequency electron-vibration interactions, leading to reduced nonradiative recombination. These findings provide insights into effectively reducing nonradiative recombination processes, thereby highlighting the potential of I−II2−III−VI4 chalcogenide compounds for high-efficiency photovoltaic applications.

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