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无铅双卤化物钙钛矿中超快自陷激子形成的时域观察

Time-Domain Observation of Ultrafast Self-Trapped Exciton Formation in Lead-Free Double Halide Perovskites.

作者信息

de Paula Ana Maria, Li Shunran, Hou Bowen, Vadivel Srikrishnaa, Teles-Ferreira Danielle C, Iudica Andrea, Kabacinski Piotr, Hosseini Hemen, McArthur Jack, Cerullo Giulio, Qiu Diana Y, Guo Peijun, Camargo Franco V A

机构信息

Departamento de Física-ICEx, Universidade Federal de Minas Gerais, 31270-901 Belo Horizonte, MG, Brazil.

Department of Chemical and Environmental Engineering, Yale University, New Haven, Connecticut 06511, United States.

出版信息

J Am Chem Soc. 2025 Aug 13;147(32):28923-28931. doi: 10.1021/jacs.5c06628. Epub 2025 Jul 30.

Abstract

Self-trapped excitons (STEs), which have one or both carriers spatially trapped by a lattice distortion, are associated with broadband emission and a large Stokes shift that is desirable for many applications. The fundamental physical processes that lead to their formation are difficult to observe, mainly due to the ultrafast time scales involved and the low oscillator strength of STE transitions. Here, we employ ultrafast transient absorption spectroscopy with sub-20 fs temporal resolution in the ultraviolet to study the STE formation process in a pair of lead-free double perovskites, CsAgInCl and Cs(AgNa)InCl. Using first-principles calculations, we assign a broad photoinduced absorption band in CsAgInCl to an intraband transition in the valence band that tracks the initial 70 fs hot-hole cooling step. Furthermore, exciton-phonon coupling calculations unravel the phonon modes that couple strongly with excitons in the lowest absorption peak to cause self-trapping. The transient absorption data shows the buildup of a stimulated emission band from the STE on a 200 fs time scale and long-lived coherent oscillations corresponding to the phonons of the lattice modified by the STE formation process.

摘要

自陷激子(STE),其一个或两个载流子在空间上被晶格畸变捕获,与宽带发射和大斯托克斯位移相关,这在许多应用中是很理想的。导致其形成的基本物理过程很难观察到,主要是由于所涉及的超快时间尺度以及STE跃迁的低振子强度。在这里,我们采用在紫外区域具有亚20飞秒时间分辨率的超快瞬态吸收光谱来研究一对无铅双钙钛矿CsAgInCl和Cs(AgNa)InCl中的STE形成过程。通过第一性原理计算,我们将CsAgInCl中一个宽的光致吸收带归因于价带中的带内跃迁,该跃迁跟踪最初70飞秒的热空穴冷却步骤。此外,激子 - 声子耦合计算揭示了在最低吸收峰中与激子强烈耦合以导致自陷的声子模式。瞬态吸收数据显示了在200飞秒时间尺度上来自STE的受激发射带的积累以及与由STE形成过程修改的晶格声子相对应的长寿命相干振荡。

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