Isothermal section of the Ho–Cu–Sn ternary system at 670 K

Author:

Romaka L.,Romaniv I.,Romaka V.,Konyk M.,Horyn A.,Stadnyk Yu.

Abstract

The interaction of the components in the Ho-Cu-Sn ternary system was investigated at 670 K over the whole concentration range using X-ray diffraction and EPM analyses. Four ternary compounds were formed in the Ho–Cu–Sn system at 670 K: HoCuSn (LiGaGe type, space group P63mc), Ho3Cu4Sn4 (Gd3Cu4Ge4-type, space group Immm), HoCu5Sn (CeCu5Au-type, space group Pnma), and Ho1.9Cu9.2Sn2.8 (Dy1.9Cu9.2Sn2.8-type, space group P63/mmc). The formation of the interstitial solid solution based on HoSn2 (ZrSi2-type) binary compound up to 5 at. % Cu was found.

Publisher

Vasyl Stefanyk Precarpathian National University

Subject

Physical and Theoretical Chemistry,Condensed Matter Physics,General Materials Science

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The Gd3Cu4Ge4 type – Structure–property relations;Handbook on the Physics and Chemistry of Rare Earths;2023

2. Phase equilibria in Ho-Fe-Sn ternary system at 670 K;Physics and Chemistry of Solid State;2020-06-15

3. Lu-V-{Ge, Sn} ternary systems;PHYS CHEM SOLID STAT;2019

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