Xiaotong Li (113048)Justin Hoffman (578062)Weijun Ke (1591930)Michelle Chen (740258)Hsinhan Tsai (1663324)Wanyi Nie (1477036)Aditya D. Mohite (1282425)Mikaël Kepenekian (1454509)Claudine Katan (1299831)Jacky Even (1299828)Michael R. Wasielewski (1268283)Constantinos C. Stoumpos (1364667)Mercouri G. Kanatzidis (1350288)
Low-dimensional\nhalide perovskites have recently attracted intense\ninterest as alternatives to the three-dimensional (3D) perovskites\nbecause of their greater tunability and higher environmental stability.\nHerein, we present the new homologous 2D series (NH<sub>3</sub>C<sub><i>m</i></sub>H<sub>2<i>m</i></sub>NH<sub>3</sub>)(CH<sub>3</sub>NH<sub>3</sub>)<sub><i>n</i>−1</sub>Pb<sub><i>n</i></sub>I<sub>3<i>n</i>+1</sub> (<i>m</i> = 4–9; <i>n</i> = 1–4), where <i>m</i> represents the carbon-chain number and <i>n</i> equals layer-thickness number. Multilayer (<i>n</i> >\n1) 2D perovskites incorporating diammonium cations were successfully\nsynthesized by the solid-state grinding method for <i>m</i> = 4 and 6 and by the solution method for <i>m</i> = 7–9.\nStructural characterization by single-crystal X-ray diffraction for\nthe <i>m</i> = 8 and <i>m</i> = 9 series (<i>n</i> = 1–4) reveals that these compounds adopt the <i>Cc</i> space group for even <i>n</i> members and <i>Pc</i> for odd <i>n</i> members. The optical bandgaps\nare 2.15 eV for two-layer (<i>n</i> = 2), 2.01 eV for three-layer\n(<i>n</i> = 3), and 1.90 eV for four-layer (<i>n</i> = 4). The materials exhibit excellent solution processability, and\ncasting thin-films of the <i>n</i> = 3 members was successfully\naccomplished. The films show a clear tendency for the higher-<i>m</i> members to have preferred orientation on the glass substrate,\nwith <i>m</i> = 8 exhibiting almost perfect vertical layer\norientation and <i>m</i> = 9 displaying both vertical and\nparallel layer orientation, as confirmed by grazing-incidence wide-angle\nX-ray scattering (GIWAXS) measurements. The vertical layer orientation\nfor the (NH<sub>3</sub>C<sub>8</sub>H<sub>16</sub>NH<sub>3</sub>)(CH<sub>3</sub>NH<sub>3</sub>)<sub>2</sub>Pb<sub>3</sub>I<sub>10</sub> member\nresults in the best thermal, light, and air stability within this\nseries, thus showing excellent potential for solar cell applications.
Duyen H. Cao (1350285)Peijun Guo (1410727)Arun Mannodi-Kanakkithodi (1611505)Gary P. Wiederrecht (1261458)David J. Gosztola (1343949)Nari Jeon (1437139)Richard D. Schaller (1287636)Maria K. Y. Chan (1539340)Alex B. F. Martinson (1343955)
DuyenH. Cao (1578649)Constantinos C. Stoumpos (1364667)Takamichi Yokoyama (1752223)Jenna L. Logsdon (3607061)Tze-Bin Song (1288428)Omar K. Farha (1301625)Michael R. Wasielewski (1268283)Joseph T. Hupp (1270782)Mercouri G. Kanatzidis (1350288)
Lin Li (28817)Shujuan Han (1705468)Binghua Lei (2128390)Xiaoyu Dong (734222)Hongping Wu (1568653)Zhongxiang Zhou (2034859)Zhihua Yang (47183)Shilie Pan (1431682)
Natalia B. Shustova (1464106)Igor V. Kuvychko (2227720)Robert D. Bolskar (2377267)Konrad Seppelt (1469203)Steven H. Strauss (1298514)Alexey A. Popov (1278525)Olga V. Boltalina (1298520)
Zarifeh Heidary (8816675)Jafar Ghaisari (8816678)Shiva Moein (8816681)Shaghayegh Haghjooy Javanmard (8816684)