Wan Xian-Kai, Han Xu-Shuang, Guan Zong-Jie, Shi Wan-Qi, Li Jiao-Jiao, Wang Quan-Ming
Department of Chemistry, Key Laboratory of Organic Optoelectronics and Molecular Engineering of the Ministry of Education, Tsinghua University, Beijing, PR China.
Key Laboratory of Green Chemistry and Technology of Ministry of Education, College of Chemistry, Sichuan University, Chengdu, Sichuan, PR China.
Nat Commun. 2024 Aug 22;15(1):7214. doi: 10.1038/s41467-024-51642-w.
It is challenging to attain strong near-infrared (NIR) emissive gold nanoclusters. Here we show a rod-shaped cluster with the composition of Au(p-MBT)(Hdppa) (1 for short, Hdppa is N,N-bis(diphenylphosphino)amine, p-MBT is 4-methylbenzenethiolate) has been synthesized. Single crystal X-ray structural analysis reveals that it has a rod-like face-centered cubic (fcc) Au kernel built from two interpenetrating bicapped cuboctahedral Au units. 1 features NIR luminescence with an emission maximum at 920 nm, and the photoluminescence quantum yield (PLQY) is 12%, which is 30-fold of [Au(m-MBT)(Hdppa)]SOCF (2, m-MBT is 3-methylbenzenethiolate) with a similar composition and 60-fold of AuS(S‑t‑Bu) with a similar structure. time-dependent DFT(TDDFT)calculations reveal that the luminescence of 1 is associated with the Au kernel. The small Stokes shift of 1 indicates that it has a very small excited state structural distortion, leading to high radiative decay rate (k) probability. The emission of cluster 1 is a mixture of phosphorescence and thermally activated delayed fluorescence(TADF), and the enhancement of the NIR emission is mainly due to the promotion of k rather than the inhibition of k. This work demonstrates that the metal kernel and the surface structure are both very important for cluster-based NIR luminescence materials.
获得强近红外(NIR)发射的金纳米团簇具有挑战性。在此,我们展示了一种组成式为Au(p-MBT)(Hdppa)(简称为1,Hdppa为N,N-双(二苯基膦基)胺,p-MBT为4-甲基苯硫醇盐)的棒状团簇已被合成。单晶X射线结构分析表明,它具有由两个相互贯穿的双帽立方八面体金单元构建而成的棒状面心立方(fcc)金核。1具有近红外发光,发射最大值在920 nm,光致发光量子产率(PLQY)为12%,这是具有相似组成的[Au(m-MBT)(Hdppa)]SOCF(2,m-MBT为3-甲基苯硫醇盐)的30倍,以及具有相似结构的AuS(S-t-Bu)的60倍。含时密度泛函理论(TDDFT)计算表明,1的发光与金核相关。1的小斯托克斯位移表明它具有非常小的激发态结构畸变,导致高辐射衰减率(k)概率。团簇1的发射是磷光和热激活延迟荧光(TADF)的混合,近红外发射的增强主要是由于k的促进而非k的抑制。这项工作表明,金属核和表面结构对于基于团簇的近红外发光材料都非常重要。