Characterization in the Icosahedral Phase of Al63Cu25Fe12 System

The present work aimed to characterize the microstructure of the icosahedral phase (quasicrystalline phase-ϕ) of the system with stoichiometric composition of the quasicrystal Al63Cu25Fe12. The ternary alloy with nominal composition of Al63Cu25Fe12 was processed by mechanical alloying (MA) as a viab...

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Bibliographic Details
Main Authors: Luciano Nascimento, Anastasiia Melnyk
Format: Article
Language:English
Published: Universidade Federal de Mato Grosso do Sul 2019-07-01
Series:Orbital: The Electronic Journal of Chemistry
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Online Access:https://periodicos.ufms.br/index.php/orbital/article/view/15933
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Summary:The present work aimed to characterize the microstructure of the icosahedral phase (quasicrystalline phase-ϕ) of the system with stoichiometric composition of the quasicrystal Al63Cu25Fe12. The ternary alloy with nominal composition of Al63Cu25Fe12 was processed by mechanical alloying (MA) as a viable solid state processing method for producing various metastable and stable quasicrystalline phases. The structural characterization of the obtained samples was performed by X-ray diffraction (XRD) and scanning electron microscopy (SEM), while the elemental composition was determined by dispersive energy spectroscopy (DES). The diffraction patterns of Al63Cu25Fe12 showed the presence of quasicrystalline phase-ϕ, ω-Al7Cu2Fe, β-Al(Fe, Cu) and λ-Al13Fe4 phases that coexist with the thermodynamic quasicrystalline phase-ϕ. In icosahedral phase oxidation of aluminum forms a dense layer on the passivating outer most surface of the quasicrystal which causes depletion in both copper and iron. It was observed not only the presence of alumina, γ-Al2O3, but also the formation of hematite and copper oxide in the dense layer. Finally, elemental analysis indicates that during alloy synthesis there is little variation of the ideal composition. The results indicate that alloys with high percentage of icosahedral phase can be obtained by casting in the air. DOI: http://dx.doi.org/10.17807/orbital.v11i3.1381
ISSN:1984-6428