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R15Si9C 化合物(R = Ho、Er、Tb)的晶体和磁性结构。

Crystal and magnetic structure of the R15Si9C compounds (R = Ho, Er, Tb).

机构信息

Institut Laue-Langevin, BP 156, Grenoble, France.

出版信息

J Phys Condens Matter. 2011 Jul 27;23(29):296002. doi: 10.1088/0953-8984/23/29/296002. Epub 2011 Jun 30.

DOI:10.1088/0953-8984/23/29/296002
PMID:21715952
Abstract

The synthesis of the new compounds R(15)Si(9)C with R = Sm, Gd-Er, Y and R(15)Ge(9)C with R = Ce, Pr and Nd has been recently reported; these compounds crystallize in the hexagonal La(15)Ge(9)Fe structure type, hP50-P6(3)mc, Z = 2 (ordered superstructure of La(5)Ge(3) (Mn(5)Si(3)-type, hP 16-P6(3)/mcm, Z = 2)). Here we report the results of a neutron diffraction investigation that we have performed to study the crystal and magnetic structures of the R(15)Si(9)C compounds with R = Tb, Ho and Er. All three compounds see the establishment of commensurate magnetic order with a predominantly ferromagnetic interaction. Details of mixed antiferro-ferromagnetic spin arrangements (κ = [000]) (for Tb(15)Si(9)C and Ho(15)Si(9)C) or of purely ferromagnetic ordering (Er(15)Si(9)C), and of their temperature dependence, are given and linked to the different coordination of the four dissimilar rare earth sites. In the Tb and Ho compounds the thermal evolution of the magnetic moment values strongly differs between the different R sites. The position occupied by the principal carbon has been determined (Wyckoff site 2b) and the existence of a second position available for the interstitial carbon (Wyckoff site 2a) has been revealed for R = Ho, Tb. Moreover, in the Tb and Ho compounds the magnetic moment value of the rare earth site R4, surrounding the second interstitial carbon site, is strongly reduced if compared to the value on the other rare earth sites. The magnetic transition temperatures of all three compounds, i.e. T(C) = 130, 43 and 45 K for Tb(15)Si(9)C, Ho(15)Si(9)C and Er(15)Si(9)C, are remarkably high compared to those of the parent R(5)Si(3) compounds. The magnetic behaviour of the partly filled Tb(5)Si(3)C(0.25) is reported.

摘要

新化合物 R(15)Si(9)C(其中 R = Sm、Gd-Er、Y)和 R(15)Ge(9)C(其中 R = Ce、Pr 和 Nd)的合成最近已有报道;这些化合物结晶于六方 La(15)Ge(9)Fe 结构类型,hP50-P6(3)mc,Z = 2(有序超结构 La(5)Ge(3)(Mn(5)Si(3)型,hP 16-P6(3)/mcm,Z = 2))。在这里,我们报告了我们进行的中子衍射研究的结果,该研究旨在研究 R(15)Si(9)C 化合物(其中 R = Tb、Ho 和 Er)的晶体和磁结构。这三种化合物均建立了具有主要铁磁相互作用的准同型磁有序。给出了混合反铁磁-铁磁自旋排列(κ = [000])(对于 Tb(15)Si(9)C 和 Ho(15)Si(9)C)或纯铁磁有序(Er(15)Si(9)C)的细节,以及它们的温度依赖性,并将其与四个不同的稀土位点的不同配位联系起来。在 Tb 和 Ho 化合物中,不同 R 位点的磁矩值的热演化有很大差异。已确定主要碳的位置(Wyckoff 位 2b),并揭示了对于 Ho、Tb 而言,第二个间隙碳位置可用(Wyckoff 位 2a)。此外,在 Tb 和 Ho 化合物中,围绕第二个间隙碳位置的 R4 稀土位点的磁矩值与其他稀土位点相比大大降低。所有三种化合物的磁转变温度,即 T(C) = 130、43 和 45 K 对于 Tb(15)Si(9)C、Ho(15)Si(9)C 和 Er(15)Si(9)C,与母体 R(5)Si(3)化合物相比非常高。报告了部分填充的 Tb(5)Si(3)C(0.25)的磁行为。

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