J. Mater. Sci. Technol. ›› 2026, Vol. 241: 1-17.DOI: 10.1016/j.jmst.2025.03.072

• Research Article •     Next Articles

Precipitation behavior and mechanical properties of 16Cr-25Ni austenitic stainless steel weld metals with different Mo content during aging

Chenghao Liua,b, Jian Suna,*, Shanping Lua,*   

  1. aShenyang National Laboratory for Materials Science, Institute of Metal Research, Chinese Academy of Sciences, Shenyang 110016, China;
    bSchool of Materials Science and Engineering, University of Science and Technology of China, Shenyang 110016, China
  • Received:2024-12-23 Revised:2025-02-24 Accepted:2025-03-24 Published:2026-01-10 Online:2025-05-11
  • Contact: *E-mail addresses: jsun16b@imr.ac.cn (J. Sun), shplu@imr.ac.cn (S. Lu)

Abstract: In this work, 16Cr-25Ni austenitic stainless steel weld metals (WM) were prepared with Mo contents of 6.3 wt.% and 2.4 wt.%. The evolution of precipitates and their influence on the impact fracture behavior of two WMs under as-weld, post-weld heat treatment (PWHT), and aging after PWHT conditions were systematically studied. The results showed that the reduction of Mo content changed the precipitation behavior of precipitated phases in the WMs. The 6.3 wt.% Mo WM contained M6C carbides, M23C6 carbides, and M2(C, N) carbonitrides. However, only the M23C6 carbides were present in the 2.4 wt.% Mo WM. The M6C carbides remained stable in the interdendritic regions (IDRs) of the 6.3 wt.% Mo WM for aging 5000 h after PWHT. The M23C6 carbides and M2(C, N) carbonitrides aggregated in IDRs. Additionally, approximately 71 nm of M23C6 carbides precipitated semi-continuously along the grain boundaries (GBs). In the 2.4 wt.% Mo WM for aging 5000 h after PWHT, M23C6 carbides were distributed in the IDRs and dendrite core regions (DCRs). Along the GBs, continuous M23C6 precipitates about 252 nm in size were observed. As the Mo content of the WM decreased, the tensile strength decreased slightly, but its impact toughness increased significantly under different conditions. During the impact of the WMs, deformation twins, deformation bands, dislocation slip, and secondary phases interacted to influence impact toughness. Deformation twins and deformation bands contributed to the impact toughness of the WMs. However, the number of deformation twins in the 2.4 wt.% Mo WM was always higher than that in the 6.3 wt.% Mo WM. For aging 5000 h after PWHT, micron-size M6C carbides caused crack initiation, and nano-size M23C6 carbides and M2(C, N) carbonitrides clusters in the IDRs of the 6.3 wt.% Mo WM strongly impeded dislocations, making IDRs preferred paths for crack propagation. In the 2.4 wt.% Mo WM, M23C6 along GBs provided significant dislocation pinning. This caused GBs to be the primary crack initiation and propagation paths.

Key words: Mo content, Austenitic stainless steel weld metals, Aging, Microstructural evolution, Impact toughness