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FeNi-based alloys are known to crystallize in bcc or fcc-structures depending on their composition. In many slowly cooled objects, like meteorites, L10-type phase (tetrataenite) with its characteristic layered Fe/Ni structure has been found. Nevertheless, the synthesis of L10 FeNi phase in industrial amount in a bulk form has not been possible, mainly due to sluggish diffusion and low order/disorder temperature of this phase. We present results of the calculations of formation enthalpies for solid solution and amorphous phase in Fe-Ni system. Additionally, we performed calculations for Co and Cu substitutions (found in meteoritic matter). Our calculations confirm poor glass forming ability of FeNi system and limited influence of Co in this aspect. In contrast, Cu is a promising candidate when aiming at destabilization of FeNi solid solution, as a starting point in L10 phase formation. Formation enthalpy for some Cu-substituted compositions reaches highly negative values. It is expected that at least local chemical segregation should be facilitated by the presence of Cu atoms (attributed mainly to different values of Cu-Co and Cu-Ni interfacial enthalpies).
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Kołodziej et al. (2022) studied this question.
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