Effect of tungsten concentration on microstructures of Co-10Ni-6Al-(0,2,4,6)W-6Ti (at%) cobalt-based superalloys

Abstract

The effects of reducing the W concentration (and concomitantly mass density) of Co-10Ni-6Al-xW-6Ti at% Co-based superalloys, with a γ(f.c.c.) plus γ′(L12) microstructure, is investigated for a series of alloys with W concentrations of 6at% (baseline alloy), 4 and 2at% (W-reduced) and 0at% (W-free). The γ′(L12) solvus temperature decreases strongly (by 46°C per 1at% reduction in W), while the liquidus and solvus temperatures decrease mildly (3–5°C per 1at% W reduction) as measured by differential scanning calorimetry. Scanning electron microscopy was used to image phase formation in all alloys. When aging at 900 or 1000°C for 256h, the W reduction does not result in the appearance of additional phases within the grains beyond the γ(f.c.c.) and γ′(L12) phases present in the original alloy. Grain-boundary precipitates are present for all alloy compositions: W-rich or W-free precipitates after aging at 1000°C, and coarsened γ′(L12) precipitates after aging at 900°C. The composition of grain boundary precipitates were measured with energy-dispersive X-ray spectroscopy. Vickers microhardness values decrease with decreasing W content, due to a reduction in γ′(L12) precipitation and reduced solid-solution strengthening.