Abstract

Nanostructured semiconductors emit light from electronic states known as excitons. For organic materials, Hund's rules state that the lowest-energy exciton is a poorly emitting triplet state. For inorganic semiconductors, similar rules predict an analogue of this triplet state known as the 'dark exciton'. Because dark excitons release photons slowly, hindering emission from inorganic nanostructures, materials that disobey these rules have been sought. However, despite considerable experimental and theoretical efforts, no inorganic semiconductors have been identified in which the lowest exciton is bright. Here we show that the lowest exciton in caesium lead halide perovskites (CsPbX3, with X = Cl, Br or I) involves a highly emissive triplet state. We first use an effective-mass model and group theory to demonstrate the possibility of such a state existing, which can occur when the strong spin-orbit coupling in the conduction band of a perovskite is combined with the Rashba effect. We then apply our model to CsPbX3 nanocrystals, and measure size- and composition-dependent fluorescence at the single-nanocrystal level. The bright triplet character of the lowest exciton explains the anomalous photon-emission rates of these materials, which emit about 20 and 1,000 times faster than any other semiconductor nanocrystal at room and cryogenic temperatures, respectively. The existence of this bright triplet exciton is further confirmed by analysis of the fine structure in low-temperature fluorescence spectra. For semiconductor nanocrystals, which are already used in lighting, lasers and displays, these excitons could lead to materials with brighter emission. More generally, our results provide criteria for identifying other semiconductors that exhibit bright excitons, with potential implications for optoelectronic devices.

Highlights

  • For organic materials, Hund’s rules[2] state that the lowest energy exciton is a poorly emitting triplet state

  • We first use the effective-mass model and group theory to explore this possibility, which can occur when the strong spin–orbit coupling in the perovskite conduction band is combined with the Rashba effect[5,6,7,8,9,10]

  • The bright-triplet exciton is further confirmed by detailed analysis of the fine structure in low-temperature fluorescence spectra

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Summary

Bright triplet excitons in lead halide perovskites

If the effective Rashba field is parallel to one of the orthorhombic symmetry axes of the nanocrystal (see Supplementary Section 1 for details and other cases), the bright triplet exciton (J=1) is split into three nondegenerate sublevels:. Because the nanocrystal size and aB are comparable, the electron and hole motion is correlated If this effect is added (intermediate exciton confinement, blue circles), calculations for L~4-16 nm (Supplementary Section 3 and Extended Data Fig. 8) agree well with experiment. Band-edge sublevels are bright, and these can be poorly populated even at room temperature This and other effects (Supplementary Section 5) explain why room-temperature emission from CsPbX3 perovskite nanocrystals is 20x faster than in other systems. G., Nedelcu, G., Protesescu, L., Bodnarchuk, M. Single cesium lead halide perovskite nanocrystals at low temperature: Fast singlephoton emission, reduced blinking, and exciton fine structure.

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