The Lutetium-rich Indide Lu13Ni6In

被引:8
作者
Galadzhun, Yaroslav V. [1 ,2 ]
Hoffmann, Rolf-Dieter [2 ]
Heletta, Lukas [2 ]
Horiacha, Myroslava [2 ,3 ]
Poettgen, Rainer [2 ]
机构
[1] Ivan Franko Natl Univ Lviv, Dept Life Safety, Doroshenka St 41, UA-79000 Lvov, Ukraine
[2] Univ Munster, Inst Anorgan & Analyt Chem, Corrensstr 30, D-48149 Munster, Germany
[3] Ivan Franko Natl Univ Lviv, Inorgan Chem Dept, Kyryla & Mephodiya St 6, UA-79005 Lvov, Ukraine
来源
ZEITSCHRIFT FUR ANORGANISCHE UND ALLGEMEINE CHEMIE | 2018年 / 644卷 / 22期
关键词
Indide; Lutetium; Nickel; Superstructure; Structure elucidation; COMPUTER-PROGRAM; CRYSTAL; RE; GD; TM; HO;
D O I
10.1002/zaac.201800188
中图分类号
O61 [无机化学];
学科分类号
070301 ; 081704 ;
摘要
The lutetium-rich indide Lu13Ni6In was synthesized from the elements by arc-melting and subsequent annealing in a sealed niobum container. At room temperature, the Lu13Ni6In structure is centrosymmetric, space group R3m, a = 919.74(10), c = 1828.9(2) pm, wR(2) = 0.0996, 666 F-2 values, 43 variables. It exhibits strong anisotropic displacement parameters U-33 for the Lu1 and U-22 for the Ni atoms. In going to low-temperature, Lu13Ni6In shows a phase transition (loss of the inversion symmetry) along with an ordering of Lu1. The structure was refined from 90 K single-crystal X-ray diffractometer data for an inversion twin: R3m, a = 918.97(4), c = 1820.27(7) pm, wR(2) = 0.0890, 1288 F-2 values, 56 variables. The low-temperature Lu13Ni6In structure can be described as a condensation of In@Lu-12 icosahedra, Ni2@Lu-6 trigonal prisms, and Ni@Lu-4 tetrahedra to layers that are stacked in ABC sequence. The driving force for superstructure formation is a strengthening of Lu-Ni bonding. Temperature dependent magnetic susceptibility measurements show Pauli paramagnetic behavior.
引用
收藏
页码:1513 / 1518
页数:6
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