New Selenites: Hydrothermal Syntheses, Crystal Structures, and Characterization of Rb3HGa2(OH)2(SeO3)4, Rb3Ga5(SeO3)8(HSeO3)2·0.5H2O, and RbGa(SeO3)2·H2O

2013 ◽  
Vol 52 (17) ◽  
pp. 10080-10086 ◽  
Author(s):  
Dong Woo Lee ◽  
Kang Min Ok
2003 ◽  
Vol 18 (2) ◽  
pp. 128-134 ◽  
Author(s):  
A. Le Bail ◽  
A.-M. Mercier

The crystal structures of the chiolite-related room temperature phases α-Na5M3F14 (MIII=Cr,Fe,Ga) are determined. For all of them, the space group is P21/n, Z=2; a=10.5096(3) Å, b=7.2253(2) Å, c=7.2713(2) Å, β=90.6753(7)° (M=Cr); a=10.4342(7) Å, b=7.3418(6) Å, c=7.4023(6) Å, β=90.799(5)° (M=Fe), and a=10.4052(1) Å, b=7.2251(1) Å, c=7.2689(1), β=90.6640(4)° (M=Ga). Rietveld refinements produce final RF factors 0.036, 0.033, and 0.035, and RWP factors, 0.125, 0.116, and 0.096, for MIII=Cr, Fe, and Ga, respectively. The MF6 polyhedra in the defective isolated perovskite-like layers deviate very few from perfect octahedra. Subtle octahedra tiltings lead to the symmetry decrease from the P4/mnc space group adopted by the Na5Al3F14 chiolite aristotype to the P21/n space group adopted by the title series. Facile twinning precluded till now the precise characterization of these compounds.


CrystEngComm ◽  
2009 ◽  
Vol 11 (11) ◽  
pp. 2431 ◽  
Author(s):  
Jonna Jokiniemi ◽  
Jouko Vepsäläinen ◽  
Harri Nätkinniemi ◽  
Sirpa Peräniemi ◽  
Markku Ahlgrén

2009 ◽  
Vol 182 (4) ◽  
pp. 913-919 ◽  
Author(s):  
Xin Wang ◽  
Tian-Lu Sheng ◽  
Sheng-Min Hu ◽  
Rui-Biao Fu ◽  
Jian-Shan Chen ◽  
...  
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