Microstructure of Precipitation Hardenable Powder Metallurgical Ni Alloys Containing 35 to 45 pct Cr and 3.5 to 6 pct Nb

Ni-based alloys with high Cr contents are not only known for their excellent high temperature and hot corrosion resistance, but are also known for poor mechanical properties and difficult workability. Powder metallurgical (PM) manufacturing of alloys may overcome several of the shortcomings encountered in materials manufacturing involving solidification. In the present work, six PM Ni-based alloys containing 35 to 45 wt pct Cr and 3.5 to 6 wt pct Nb were produced and compacted via hot isostatic pressing. Samples were heat treated for up to 1656 hours at either 923 K or 973 K (650 A degrees C or 700 A degrees C), and the microstructures and mechanical properties were quantified and compared to thermodynamic calculations. For the majority of the investigated alloys, the high Cr and Nb contents caused development of primary populations of globular alpha-Cr and delta (Ni3Nb). Transmission electron microscopy of selected alloys confirmed the additional presence of metastable gamma aEuro(3) (Ni3Nb). A co-dependent growth morphology was found, where the preferred growth direction of gamma aEuro(3), the {001} planes of gamma-Ni, caused precipitates of both alpha-Cr and delta to appear in the form of mutually perpendicular oriented disks or plates. Solution heat treatment at 1373 K (1100 A degrees C) followed by aging at 973 K (700 A degrees C) produced a significant strength increase for all alloys, and an aged yield strength of 990 MPa combined with an elongation of 21 pct is documented for Ni 40 wt pct Cr 3.5 wt pct Nb.