“…[10,11] The degradation is summarized as follows. Z phase forms in ferritic/martensitic steels containing large amounts of Cr and N, V, and Nb after long thermal exposure similar to the case for austenitic steel; [26,30] the nose temperature of Z-phase precipitation (i.e., the temperature at which precipitation occurs earliest) is 923 K (650°C); [27] the composition of Z phase is Cr(Nb,V)N, and small amounts of Fe and Si are dissolved; [27,28] a thermodynamic calculation system showed that Z phase is more stable than MX in high-Cr ferritic/martensitic steel; [30][31][32] the nucleation mechanism is not well understood, but Z phase easily nucleates on VN and Z phase is further stabilized by dissolving Nb; [32][33][34] Nb precipitates forming MX on PAGB during normalization, and Z phase is found on PAGB near Nb containing MX; [28,35,36] Z-phase particles grow and/or become coarse by collecting nearby Cr, and dissolving and consuming finely dispersed MX particles in grains [35,36] ; and a region several microns in width along and adjacent to PAGB on which coarse M 23 C 6 and Z-phase particles grow is preferentially recovered, the timing of which corresponds to an unexpected and sharp drop in strength. [10,[35][36][37] According to the previous work shown above, the unexpected drop in strength in the times to rupture and specified strain observed at 873 K (600°C) after several thousands of hours for 11Cr-2W-0.4Mo-1Cu-Nb-V steel (shown in Figures 2, 7, and 11) is considered to be mainly because of the formation of Z phase on PAGB and the resulting local and heterogeneous recovery along PAGB.…”