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Mechanism of hot ductility loss in C–Mn steels based on nonequilibrium grain boundary segregation of impurities

Published online by Cambridge University Press:  24 April 2015

Zongwen Zheng*
Affiliation:
Superalloy Department, Central Iron & Steel Research Institute, Beijing 100081, People's Republic of China
Hongyao Yu
Affiliation:
Superalloy Department, Central Iron & Steel Research Institute, Beijing 100081, People's Republic of China
Zhenjun Liu
Affiliation:
Superalloy Department, Central Iron & Steel Research Institute, Beijing 100081, People's Republic of China
Tingdong Xu
Affiliation:
Superalloy Department, Central Iron & Steel Research Institute, Beijing 100081, People's Republic of China
R. Devesh K. Misra
Affiliation:
Department of Metallurgical and Materials Engineering, Center for Structural and Functional Materials Research and Innovation, University of Texas at El Paso, El Paso, Texas 79968, USA
*
a) Address all correspondence to this author. e-mail: zwzheng2013@163.com

Abstract

The subject of hot ductility in C–Mn steels has been the focus of interest for a long time in materials science and engineering. However, the mechanism of loss in hot ductility continues to be unclear. In the present paper, the experimental hot ductility data in C–Mn steels involve: (i) a ductility trough appears at a certain temperature when the sample is held for a certain time at various temperatures after cooling quickly from a higher temperature; (ii) the ductility healing phenomenon which occurs with the duration of holding time; (iii) the ductility deteriorates with the increase of temperature difference between solution treatment temperature and test temperature during a tensile test; (iv) a minimum ductility appears when samples are cooled from a higher temperature to a lower one at a certain cooling rate; and (v) the formation of cavities at grain boundaries during tests. All of these are analyzed and calculated from the perspective of thermally induced nonequilibrium grain-boundary segregation (TNGS). Based on our detailed analyses, the loss in hot ductility of C–Mn steels is ascribed to TNGS of impurities.

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Copyright © Materials Research Society 2015 
Figure 0

FIG. 1. (a) Influence of TT and sulfur content on RA at a RHT of 1573 K for Ht of 300 s. (b) Influence of Ht on RA for steel 10. RHT and TT are 1573 and 1223 K, respectively.29

Figure 1

TABLE I. The parameters used for calculations.

Figure 2

FIG. 2. The isothermal kinetics of S TNGS in C–Mn steel calculated with Eqs. (1)–(4) for holding at 1123, 1173, 1223, 1273, and 1323 K after cooling from 1573 K.

Figure 3

TABLE II. The critical time calculated at different holding temperatures.

Figure 4

FIG. 3. TNGS concentrations of S in C–Mn steel held for 300 s at 1123, 1173, 1223, 1273, and 1323 K, respectively, after cooling from 1573 K.

Figure 5

FIG. 4. Hot ductility plots of the as-cast and as-rolled C–Mn steels after reheating treatment at 1330 °C.41

Figure 6

FIG. 5. (a) Hot ductility of steels 1 and 2 as a function of TT. (b) Isothermal hot ductility change in steel 2 at different TTs after solution treatment at 1250 °C in Kobayashi's study.43

Figure 7

FIG. 6. Influence of RHT on RA at the tensile TT of 1223 K for a Ht of 300 s in 0.014–0.017 wt% sulfur steels.29

Figure 8

FIG. 7. The relationship between the RHT and the maximum concentration of S TNGS.

Figure 9

FIG. 8. Hot ductility with various thermal histories for C–Mn steels.5

Figure 10

FIG. 9. Effect of cooling rate on the hot ductility of steels 3 and 4 in Kobayashi's study.43

Figure 11

FIG. 10. Variation of RA with cooling rate from solution-treated temperature to TT of tensile test, for two C–Mn steels solution treated at 1350 °C and tested at 1050 °C.42

Figure 12

FIG. 11. The calculated results of the effective time of sulfur in C–Mn steel at 1050 °C with different cooling rates.

Figure 13

FIG. 12. (a) Effect of cooling rate on the hot ductility of the Sn-doped steel. (b) The grain boundary concentration of Sn in specimens cooled at different cooling rates, determined by AES (bars represent standard deviation).32

Figure 14

FIG. 13. SEM micrographs of the intergranular ruptured surface at a RA of 3% for C–Mn steel. RHT, TT, and Ht are 1573, 1273 K, and 300 s, respectively.29