TY - JOUR
T1 - Aging 17-4 PH martensitic stainless steel prior to hardening
T2 - effects on martensitic transformation, microstructure and properties
AU - Villa, Matteo
AU - Grumsen, Flemming B.
AU - Niessen, Frank
AU - Dahmen, Thomas
AU - Cao, Lingfei
AU - Reich, Michael
AU - Kessler, Olaf
AU - Huang, Xiaoxu
AU - Somers, Marcel A.J.
N1 - Publisher Copyright:
© 2023 The Authors
PY - 2023
Y1 - 2023
N2 - Precipitation hardening martensitic stainless steel 17-4 PH is conventionally austenitized and air cooled to room temperature to form martensite. On aging the martensitic condition tiny Cu-rich precipitates are formed that provide high strength. In the present investigation, the steel was aged in austenitic condition prior to martensite formation. Dilatometry, transmission electron microscopy, atomic probe tomography, synchrotron X-Ray diffraction, electron backscatter diffraction, hardness tests and tensile tests were applied to study austenite aging and its effects on: (i) the subsequent transformation of austenite into martensite, (ii) the microstructure of the forming martensite and (iii) the mechanical properties of the material. Austenite aging favors early formation of Cu clusters followed by precipitation of Cu particles. The evolution of the Cu precipitate size with aging time follows traditional Ostwald ripening kinetics which is rate controlled by Cu diffusion in austenite. Austenite aging affects the kinetics of martensite formation and the substructure of the martensite laths; overall, it provides significant strengthening to the martensitic material. The contribution of precipitates to the strength of martensite is interpreted in terms of the Russell-Brown model for modulus strengthening. The data and the model are reconciled by re-evaluating the adjustable parameter used in the original work. Finally, the work reports the influence of austenite aging on the mechanical properties of the material when this is further aged to peak strength in martensitic condition.
AB - Precipitation hardening martensitic stainless steel 17-4 PH is conventionally austenitized and air cooled to room temperature to form martensite. On aging the martensitic condition tiny Cu-rich precipitates are formed that provide high strength. In the present investigation, the steel was aged in austenitic condition prior to martensite formation. Dilatometry, transmission electron microscopy, atomic probe tomography, synchrotron X-Ray diffraction, electron backscatter diffraction, hardness tests and tensile tests were applied to study austenite aging and its effects on: (i) the subsequent transformation of austenite into martensite, (ii) the microstructure of the forming martensite and (iii) the mechanical properties of the material. Austenite aging favors early formation of Cu clusters followed by precipitation of Cu particles. The evolution of the Cu precipitate size with aging time follows traditional Ostwald ripening kinetics which is rate controlled by Cu diffusion in austenite. Austenite aging affects the kinetics of martensite formation and the substructure of the martensite laths; overall, it provides significant strengthening to the martensitic material. The contribution of precipitates to the strength of martensite is interpreted in terms of the Russell-Brown model for modulus strengthening. The data and the model are reconciled by re-evaluating the adjustable parameter used in the original work. Finally, the work reports the influence of austenite aging on the mechanical properties of the material when this is further aged to peak strength in martensitic condition.
KW - Austenite aging
KW - Martensitic transformation
KW - Modulus hardening
KW - Precipitation hardening
KW - Stainless steel
KW - Transformation kinetics
U2 - 10.1016/j.mtla.2023.101882
DO - 10.1016/j.mtla.2023.101882
M3 - Journal article
AN - SCOPUS:85170427538
SN - 2589-1529
VL - 32
JO - Materialia
JF - Materialia
M1 - 101882
ER -