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

  • L. Romaka Ivan Franko L’viv National University
  • I. Romaniv Ivan Franko National University of Lviv
  • V. Romaka Lviv Polytechnic National University
  • M. Konyk Ivan Franko National University of Lviv
  • A. Horyn Ivan Franko National University of Lviv
  • Yu. Stadnyk Ivan Franko National University of Lviv
Keywords: Intermetallics, Phase diagrams, X-ray diffraction, Crystal structure

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.

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Published
2019-05-02
How to Cite
[1]
RomakaL., RomanivI., RomakaV., KonykM., HorynA. and StadnykY. 2019. Isothermal section of the Ho–Cu–Sn ternary system at 670 K. Physics and Chemistry of Solid State. 19, 2 (May 2019), 139-146. DOI:https://doi.org/10.15330/pcss.19.2.139-146.
Section
Review

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