A thermodynamic model of the Z-phase Cr(V, Nb)N

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    Precipitation of large Z-phase particles, Cr(V, Nb)N, replacing fine MX carbonitrides, Nb(C, N) or V(N, C), has recently been identified as a major cause for premature breakdown in long-term creep strength of a number of new 9%–12% Cr martensitic steels, especially the high Cr variants. A thermodynamic model of the Z-phase has been developed based on the regular solution model. The model predicts Z-phase to be stable and to fully replace the MX particles in most of the new 9%–12% Cr steels, which is in good agreement with experimental observations. The rate of precipitation of Z-phase is a crucial factor for the long-term creep stability of these steels. Driving force calculations with the model allow estimates of the influence of the individual alloying elements on the rate of Z-phase precipitation, and can thus contribute useful information for alloy design to delay and retard Z-phase precipitation. According to these calculations, particularly Cr has a strong accelerating effect on Z-phase precipitation.
    Original languageEnglish
    JournalComputer Coupling of Phase Diagrams and Thermochemistry
    Issue number4
    Pages (from-to)505-514
    Publication statusPublished - 2007


    • Z-phase
    • Thermo-Calc
    • CrNbN
    • CrVN
    • Cr(V, Nb)N


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