4.7 Article

Erbium-rich region of the ternary Er-Ni-Sb system:: Solid state phase equilibria at 1073 K and crystal structures of the new ternary compound Er5Sb3-xNix (x=0.48) and both modifications of Er5Sb3

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JOURNAL OF ALLOYS AND COMPOUNDS
卷 437, 期 1-2, 页码 133-139

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ELSEVIER SCIENCE SA
DOI: 10.1016/j.jallcom.2006.07.087

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rare-earth metal antimonide; crystal structure; phase transformations; phase equilibria; X-ray diffraction

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The solid state phase equilibria in the Er-rich region of the ternary Er-Ni-Sb system were determined at 1073 K using experimental techniques such as X-ray diffraction, scanning electron microscopy and electron probe microanalysis. In addition to the ternary phase Er5Ni2Sb previously reported, a new phase Er5Sb3-xNix (x = 0.48) was obtained, the structure, of which was solved from X-ray single crystal data: space group Pnma, a = 1.17522(3) nm, b = 0.90437(3) nm, c = 0.79144(5) nm, R-1 =0.067, wR(2) = 0.070. Moreover, for the first time, both modifications of the binary antimonide Er5Sb3 were obtained and their structures were studied front X-ray powder diffraction data. The low-temperature form belongs to the Mn5Si3 type: space group P6(3)/mcm, a = 0.88062(4) nm, c = 0.62139(9) nm, R-1 = 0.074, R-P = 0.150, while the high -temperature form exhibits the beta-Yb5Sb3 type: space group Pnma, a = 1.16897(3) nm, b = 0.91425(3) nm, c = 0.80217(2) nm, R-1 = 0.077, R-p = 0.125. According to these results, one can conclude that the substitution of antimony by nickel at 1073 Kin the ternary phase Er5Sb3-xNix tends to stabilize the P-Yb5Sb3 type. (C) 2006 Elsevier B.V. All rights reserved.

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