| Literature DB >> 31183036 |
Zhi Wang1, Hao-Tian Sun1, Mohamedally Kurmoo2, Qing-Yun Liu3, Gui-Lin Zhuang4, Quan-Qin Zhao1, Xing-Po Wang1, Chen-Ho Tung1, Di Sun1,4.
Abstract
Isomerization is highly important in all aspects of science, yet it is rarely observed in nanoscience. Here, we synthesized a unique triple core-shell Ag84 nanocluster displaying isomerism, which is controlled by differentEntities:
Year: 2019 PMID: 31183036 PMCID: PMC6520922 DOI: 10.1039/c8sc05666h
Source DB: PubMed Journal: Chem Sci ISSN: 2041-6520 Impact factor: 9.825
Scheme 1Schematic representation of the assembly and conversion of SD/Ag84a and SD/Ag84b.
Fig. 1Structures of the clusters SD/Ag84a (a) and SD/Ag84b (b). (c) The polyhedral mode showing an Ag6 octahedron (green) capped by four additional silver tetrahedra (yellow) to form the Ag10 kernel; (d) two (W7O26)10– anions wrapping an Ag10 kernel and (e) polyhedral mode showing the structure of a (W7O26)10– anion. Color labels: purple, Ag; cyan, W; yellow, S; gray, C; and red, O.
Fig. 2(a) The superposed Ag74 shells of SD/Ag84a (red) and SD/Ag84b (green). (b) The top views of silver polygons at the pole regions of SD/Ag84a (red) and SD/Ag84b (green). The top views of ligand distributions at the pole region of SD/Ag84a (c) and SD/Ag84b (d).
Fig. 3Total DOS and partial DOS of SD/Ag84a (a). Frontier molecular orbitals: HOMO–2 (b), HOMO–1 (c), HOMO (d) and LUMO (e), LUMO+1 (f) and LUMO+2 (g).
Fig. 4The UV-Vis absorption spectra of SD/Ag84a and the (iPrSAg) precursor.
Fig. 5(a) The temperature-dependent emission spectra of SD/Ag84a under 468 nm excitation. Insets: the photographs of SD/Ag84a irradiated with 365 nm UV light at 298 and 77 K. (b) The plot of temperature vs. maximum emission intensity (red line is the linear fitting in the range of 83–203 K). (c) Luminescence lifetime of SD/Ag84a recorded at 83 K (red line is the fitting curve).