Exciton Fine Structure in Perovskite Nanocrystals

• Published in: Nano letters Vol. 19; no. 6; pp. 4068 - 4077
• Main Authors: Sercel, Peter C, Lyons, John L, Wickramaratne, Darshana, Vaxenburg, Roman, Bernstein, Noam, Efros, Alexander L
• Format: Journal Article
• Language: English
• Published: United States American Chemical Society 12.06.2019
• Subjects: electron−hole exchange; Rashba effect; Exciton fine structure; lead halide perovskite; nanocrystals
• ISSN: 1530-6984; 1530-6992
• DOI: 10.1021/acs.nanolett.9b01467

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 CsPbBr3 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 CsPbBr3 NCs is opposite to what has been observed experimentally. An alternate explanation for the observed bright exciton level order in CsPbBr3 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.