Abstract
Abstract The structure of Cs3Bi2I9 has been refined to R = 0.0165 on the basis of X-ray diffraction measurements at T = 290 K (STOE IPDS diffractometer; MoKα -radiation; 296 nonequivalent reflection with I > 2σ(I)). The absorption correction was accounted for by the Gaussian method. The parameters of the hexagonal unit cell are: a = 8.409(1) Å and c = 21.243(5) Å; space group P63/mmc. The structure consists of identical perovskite-like layer fragments described by the general formula A3B2X9 (A = Cs, B = Bi, X = I) with ordered vacancies in the B-sublattice. These fragments alternate along the c-axis and are related by mirror planes which contains the shared faces of the BiI6 octahedra. The analysis of the intensities in the temperature range 288 K to 190 K indicates a reversible phase transition into a monoclinic phase at T = 218 K which is accompanied by twinning. No satellite or superstructure reflections were observed with the current resolution of the diffractometer. The X-ray results are compared wih the studies of the temperature dependence of the linear expansion coefficients, optical characteristics, and the nuclear quadrupole spectra of Cs3Bi2I9.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Zeitschrift für Kristallographie - Crystalline Materials
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
