{"title":"Effective lifetime of non‐equilibrium carriers in perovskite‐inspired Cu2AgBiI6","authors":"Zenghua Cai, Chen-Min Dai, Chunlan Ma","doi":"10.1002/pssr.202400134","DOIUrl":null,"url":null,"abstract":": Perovskite‐inspired materials are potential alternatives to lead halide perovskites, as they not only inherit the benign optoelectronic properties, but also diminish the stability and toxicity issues of lead halide perovskites. As a newly discovered perovskite‐inspired material, Cu<jats:sub>2</jats:sub>AgBiI<jats:sub>6</jats:sub> has exhibited promising potential for photovoltaic applications. However, studies on its fundamental properties related to photovoltaic performance are scarce, particularly from a theoretical perspective. Here, we systematically investigate the effective lifetime of non‐equilibrium carriers (photo‐excited charge carriers), a critical property affecting the photovoltaic performance of Cu<jats:sub>2</jats:sub>AgBiI<jats:sub>6</jats:sub>, based on the non‐adiabatic molecular dynamics simulations. We find that under the standard solar spectrum illumination, the dominant recombination mechanism affecting the effective lifetime can be band‐to‐band nonradiative decay, band‐to‐band radiative decay, or Shockey‐Read‐Hall (SRH) defect‐assisted decay. The specific mechanism is highly dependent on the radiative recombination coefficient and the density of defect recombination levels. The effective lifetime can vary from 0.1 ms to 10 ns. When considering different illumination conditions (generation rates), Auger decay can also become the dominant recombination mechanism, with the effective lifetime varying from 0.1 s to 0.1 ns. These findings could be vital for further experimental researches aimed at enhancing the power conversion efficiency of Cu<jats:sub>2</jats:sub>AgBiI<jats:sub>6</jats:sub>‐based solar devices.This article is protected by copyright. All rights reserved.","PeriodicalId":54619,"journal":{"name":"Physica Status Solidi-Rapid Research Letters","volume":"82 6 1","pages":""},"PeriodicalIF":2.5000,"publicationDate":"2024-05-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physica Status Solidi-Rapid Research Letters","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1002/pssr.202400134","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"MATERIALS SCIENCE, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
: Perovskite‐inspired materials are potential alternatives to lead halide perovskites, as they not only inherit the benign optoelectronic properties, but also diminish the stability and toxicity issues of lead halide perovskites. As a newly discovered perovskite‐inspired material, Cu2AgBiI6 has exhibited promising potential for photovoltaic applications. However, studies on its fundamental properties related to photovoltaic performance are scarce, particularly from a theoretical perspective. Here, we systematically investigate the effective lifetime of non‐equilibrium carriers (photo‐excited charge carriers), a critical property affecting the photovoltaic performance of Cu2AgBiI6, based on the non‐adiabatic molecular dynamics simulations. We find that under the standard solar spectrum illumination, the dominant recombination mechanism affecting the effective lifetime can be band‐to‐band nonradiative decay, band‐to‐band radiative decay, or Shockey‐Read‐Hall (SRH) defect‐assisted decay. The specific mechanism is highly dependent on the radiative recombination coefficient and the density of defect recombination levels. The effective lifetime can vary from 0.1 ms to 10 ns. When considering different illumination conditions (generation rates), Auger decay can also become the dominant recombination mechanism, with the effective lifetime varying from 0.1 s to 0.1 ns. These findings could be vital for further experimental researches aimed at enhancing the power conversion efficiency of Cu2AgBiI6‐based solar devices.This article is protected by copyright. All rights reserved.
期刊介绍:
Physica status solidi (RRL) - Rapid Research Letters was designed to offer extremely fast publication times and is currently one of the fastest double peer-reviewed publication media in solid state and materials physics. Average times are 11 days from submission to first editorial decision, and 12 days from acceptance to online publication. It communicates important findings with a high degree of novelty and need for express publication, as well as other results of immediate interest to the solid-state physics and materials science community. Published Letters require approval by at least two independent reviewers.
The journal covers topics such as preparation, structure and simulation of advanced materials, theoretical and experimental investigations of the atomistic and electronic structure, optical, magnetic, superconducting, ferroelectric and other properties of solids, nanostructures and low-dimensional systems as well as device applications. Rapid Research Letters particularly invites papers from interdisciplinary and emerging new areas of research.