Mechanical alloying in compositions iron–titanium–carbon (diamond)

Author:

Kovaliova S.A.1,Kiseleva T.Yu.2,Grigoreva T.F.3,Zhornik V.I.1,Devyatkina E.T.3,Vosmerikov S.V.3

Affiliation:

1. Joint Institute of Mechanical Engineering of the National Academy of Sciences of Belarus

2. Lomonosov Moscow State University

3. Institute of Solid State Chemistry and Mechanochemistry Siberian Branch of the Russian Academy of Sciences Novosibirsk

Abstract

X-ray diffraction analysis, scanning electron microscopy and M¨ossbauer spectroscopy have been applied to the study of Fe-xTi (x=20–40 wt.%), Fe/xTi-diamond and Fe–Ti–C powders structure formation under the conditions of an AGO-2 planetary ball mill. It has been shown that metals with high melting points and limited solubility under high-energy mechanical action for 20 min interact to form an alloy of nanostructured iron and grain-boundary phases similar to solid solutions of Fe(Ti), Ti(Fe) and FeTi with a total content of 22–24 %. In the Fe-20wt.%Ti composition, titanium reaches an X-ray amorphous state, and when the titanium content is above 20 wt.% 𝛼-Ti crystalline phase remains in an amount of 5–10 wt.%. When the Fe/xTi-diamond mixture is mechanically activated, composite particles with a metal matrix structure with a diamond size of 0.3–1.5 𝜇m are formed. It has been established titanium accelerates the process of grain-boundary and volumetric interaction of iron with diamond and titanium carbide. In the powder compositions under study, a solid solution is formed based on iron and TiC, Fe3C compounds with their total content: Fe/40 wt.%Ti-diamond up to 62%; Fe/TiC up to 34%. Under similar conditions in a diamond-iron mixture, the grain-boundary phases of the solid solution do not exceed 26%. The formation of graphite has not detected by X-ray diffraction.

Funder

Belarusian Republican Foundation for Fundamental Research

Ministry of Science and Higher Education of the Russian Federation

Publisher

Moscow University Press

Subject

Space and Planetary Science,General Physics and Astronomy,Astronomy and Astrophysics

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