Ternary rare-earth ruthenium and iridium germanides RE3M2Ge3 (RE=Y, Gd–Tm, Lu; M=Ru, Ir)
Graphical abstract
RE3M2Ge3 (M=Ru, Ir) adopts the Hf3Ni2Si3-type structure containing slabs built up from Ge-centred trigonal prisms.
Introduction
A rich variety of ternary rare-earth transition-metal germanides RE–M–Ge are known. Among systems with M=3d metals, the ones involving the later elements (M=Mn, Fe, Co, Ni, Cu) give rise to numerous phases, in contrast to those containing the earlier elements (M=V, Cr) [1], [2], for which the new compounds REMGe3 and RECrxGe2 have only been identified recently [3], [4], [5]. The same pattern emerges for systems with M=4d and 5d metals, in which the ones containing the precious metals (M=Ru, Os, Rh, Ir, Pd, Pt) promise to show many phases, whereas those containing the earlier elements have barely been explored [1]. Much of the interest in these germanides relates to their diverse physical properties which may prove useful in materials applications. Recent reports of such germanides containing a precious metal have been motivated by the search for new magnetocaloric (e.g., GdRu2Ge2) [6], thermoelectric (e.g., RE3M4Ge13) [7], [8], and superconducting materials (e.g., RE2Ir3Ge5) [9], [10].
We present here the elucidation of the series RE3M2Ge3 (RE=Y, Gd–Tm, Lu; M=Ru, Ir). Only a few isolated members of these series have been identified previously: Ho3Ru2Ge3 [11], [12], [13], Ho3Ir2Ge3 [14], and Lu3Ir2Ge3 [15]. The crystal structures for all remaining members for the RE3Ru2Ge3 series have now been determined, as well as for Tb3Ir2Ge3. We report electrical resistivity measurements for the RE3Ru2Ge3 series, as well as magnetic susceptibility measurements on Dy3Ru2Ge3. The nature of bonding in these compounds has been examined through band structure calculations.
Section snippets
Synthesis
Stoichiometric mixtures (0.2-g total mass) of freshly filed RE pieces (RE=Y, Gd–Tm, Lu, 99.9%, Hefa), Ru (99.95%, Cerac) or Ir powder (99.9%, Cerac), and Ge powder (99.9999%, Alfa-Aesar) were pressed into pellets, which were arc-melted in a Centorr 5TA tri-arc furnace on a water-cooled copper hearth under an argon atmosphere. To ensure homogeneity, the samples were melted twice, after which the weight loss was found to be less than 1%. The ingots were then sealed within fused-silica tubes and
Results and discussion
The ternary germanides RE3M2Ge3 (RE=Y, Gd–Tm, Lu; M=Ru, Ir) have been obtained by arc-melting reactions and determined by X-ray diffraction studies to adopt the orthorhombic Hf3Ni2Si3-type structure [24]. This structure type is a relative rare one formed mostly by silicides Zr3M2Si3 (M=Fe, Co) [24], Hf3M2Si3 (M=Fe, Co, Ni) [24], RE3Fe2Si3 (RE=Gd–Tm, Lu, Y, Sc) [25], [26], RE3Co2Si3 (RE=Tb–Tm, Lu, Y, Sc) [25], [27], Sc3Ni2Si3 [28], and Y3M2Si3 (M=Rh, Pd) [29]; and germanides Gd3Mn2Ge3 [30], RE3Fe
Conclusions
Ternary rare-earth germanides RE3M2Ge3 with the Hf3Ni2Si3-type structure have been established for M=Ru, Ir, and it will be worthwhile to attempt the preparation of the analogous series with M=Os, Rh. Although the conventional description in terms of Ge-centred RE4M2 and RE6 trigonal prisms is helpful in clarifying relationships to other structures, the alternative description that emphasizes the presence of [M2Ge3] layers is more accurate in portraying the strong covalent M–Ge bonding
Acknowledgments
This work was supported by the Natural Sciences and Engineering Research Council of Canada (NSERC).
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