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钙钛矿纳米晶体中的激子精细结构

Exciton Fine Structure in Perovskite Nanocrystals.

作者信息

Sercel Peter C, Lyons John L, Wickramaratne Darshana, Vaxenburg Roman, Bernstein Noam, Efros Alexander L

机构信息

Department of Applied Physics and Materials Science , California Institute of Technology , Pasadena , California 91125 , United States.

Center for Computational Materials Science , U.S. Naval Research Laboratory , Washington D.C. 20375 , United States.

出版信息

Nano Lett. 2019 Jun 12;19(6):4068-4077. doi: 10.1021/acs.nanolett.9b01467. Epub 2019 May 22.

Abstract

The bright emission observed in cesium lead halide perovskite nanocrystals (NCs) has recently been explained in terms of a bright exciton ground state [ Becker et al. Nature 2018 , 553 , 189 - 193 ], a claim that would make these materials the first known examples in which the exciton ground state is not an optically forbidden dark exciton. This unprecedented claim has been the subject of intense experimental investigation that has so far failed to detect the dark ground-state exciton. Here, we review the effective-mass/electron-hole exchange theory for the exciton fine structure in cubic and tetragonal CsPbBr NCs. In our calculations, the crystal field and the short-range electron-hole exchange constant were calculated using density functional theory together with hybrid functionals and spin-orbit coupling. Corrections associated with long-range exchange and surface image charges were calculated using measured bulk effective mass and dielectric parameters. As expected, within the context of the exchange model, we find an optically inactive ground exciton level. However, in this model, the level order for the optically active excitons in tetragonal CsPbBr NCs is opposite to what has been observed experimentally. An alternate explanation for the observed bright exciton level order in CsPbBr NCs is offered in terms of the Rashba effect, which supports the existence of a bright ground-state exciton in these NCs. The size dependence of the exciton fine structure calculated for perovskite NCs shows that the bright-dark level inversion caused by the Rashba effect is suppressed by the enhanced electron-hole exchange interaction in small NCs.

摘要

最近,卤化铯铅钙钛矿纳米晶体(NCs)中观察到的明亮发射现象已根据明亮激子基态得到了解释[贝克尔等人,《自然》,2018年,第553卷,第189 - 193页],这一说法将使这些材料成为激子基态不是光学禁戒暗激子的首个已知实例。这一史无前例的说法一直是深入实验研究的主题,然而迄今为止尚未检测到暗基态激子。在此,我们回顾了立方和四方CsPbBr NCs中激子精细结构的有效质量/电子 - 空穴交换理论。在我们的计算中,使用密度泛函理论结合杂化泛函和自旋轨道耦合来计算晶体场和短程电子 - 空穴交换常数。利用测量的体有效质量和介电参数计算与长程交换和表面镜像电荷相关的修正。正如预期的那样,在交换模型的框架内,我们发现了一个光学非活性的基激子能级。然而,在该模型中,四方CsPbBr NCs中光学活性激子的能级顺序与实验观察结果相反。针对CsPbBr NCs中观察到的明亮激子能级顺序,我们根据Rashba效应提供了另一种解释,该效应支持这些NCs中存在明亮基态激子。对钙钛矿NCs计算得到的激子精细结构的尺寸依赖性表明,由Rashba效应引起的明暗能级反转在小尺寸NCs中因增强的电子 - 空穴交换相互作用而受到抑制。

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