2019
DOI: 10.1002/srin.201900444
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Precipitation and Mechanical Property of V‐Alloyed Steel: Role of Cooling Rate

Abstract: Herein, the effect of cooling rate on the precipitation behavior and mechanical properties of V-added microalloyed steel is systematically investigated by nanoindentation test, X-ray diffraction, and transmission electron microscopy. The present observation reveals that random precipitates and interphase precipitates are simultaneously observed at the low cooling rate of 0.5 C s À1 , whereas only random precipitates are obtained at the high cooling rate of 2 C s À1 . The contribution of the nanoscale precipita… Show more

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Cited by 9 publications
(8 citation statements)
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“…Therefore, the classic Williamson–Hall method was recently utilized in several studies which evaluated the dislocation density of the tempered microstructure of ultrahigh strength steels. [ 45–52 ] No martensitic microstructures with the high dislocation density exist in the present steels, and their microstructure is comparable with the tempered steel consisting of fully ferritic matrix‐containing precipitates; thus, this study calculated the dislocation densities using the classic Williamson–Hall method (Equation (3))ρ=ρsρp$$\left(^{\rho = \textrm{ } \sqrt{} \rho}\right)_{\text{s}} \left(^{\rho}\right)_{\text{p}}$$where ρ s is the dislocation density calculated from strain broadening and ρ p is the dislocation density calculated from crystallite size. The following Equation (4) and (5) were used to evaluate ρ s and ρ p of the body‐centered cubic metalρs= 14.4ε2false/Fb2$$\left(\rho\right)_{\text{s}} = \textrm{ } 14.4 \left(\epsilon\right)^{2} / F b^{2}$$ρp= 3nfalse/D2$$\left(\rho\right)_{\text{p}} = \textrm{ } 3 n / D^{2}$$where ε is microstrain, b is Burgers vector, F is an interaction factor assumed to be 1, and D is crystallite size.…”
Section: Resultsmentioning
confidence: 99%
See 3 more Smart Citations
“…Therefore, the classic Williamson–Hall method was recently utilized in several studies which evaluated the dislocation density of the tempered microstructure of ultrahigh strength steels. [ 45–52 ] No martensitic microstructures with the high dislocation density exist in the present steels, and their microstructure is comparable with the tempered steel consisting of fully ferritic matrix‐containing precipitates; thus, this study calculated the dislocation densities using the classic Williamson–Hall method (Equation (3))ρ=ρsρp$$\left(^{\rho = \textrm{ } \sqrt{} \rho}\right)_{\text{s}} \left(^{\rho}\right)_{\text{p}}$$where ρ s is the dislocation density calculated from strain broadening and ρ p is the dislocation density calculated from crystallite size. The following Equation (4) and (5) were used to evaluate ρ s and ρ p of the body‐centered cubic metalρs= 14.4ε2false/Fb2$$\left(\rho\right)_{\text{s}} = \textrm{ } 14.4 \left(\epsilon\right)^{2} / F b^{2}$$ρp= 3nfalse/D2$$\left(\rho\right)_{\text{p}} = \textrm{ } 3 n / D^{2}$$where ε is microstrain, b is Burgers vector, F is an interaction factor assumed to be 1, and D is crystallite size.…”
Section: Resultsmentioning
confidence: 99%
“…Therefore, the classic Williamson-Hall method was recently utilized in several studies which evaluated the dislocation density of the tempered microstructure of ultrahigh strength steels. [45][46][47][48][49][50][51][52] No martensitic microstructures with the high dislocation density exist in the present steels, and their microstructure is comparable with the tempered steel consisting of fully ferritic matrix-containing precipitates; thus, this study calculated the dislocation densities using the classic Williamson-Hall method (Equation (3))…”
Section: Dislocation Densitymentioning
confidence: 99%
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“…When HSLA steels contain a ternary system of the abovementioned three alloy elements or a binary system in which two elements are combined, the relationship among the tempering process parameters, carbide precipitation, and performance becomes complex. [5,7,8] MX-type carbon (nitrogen) compounds with the NaCl (B1) cubic crystal structure are precipitated, such as NbC, Nb (C, N), (Ti, Nb) C, and (Ti, Nb, V)C, in the binary or ternary system of microalloy steels. In addition to MX-type precipitation, M 3 C, M 2 C, M 23 C 6 , and M 7 C 3 precipitates [7,9,10] cause the carbides in HSLA steels to exhibit the characteristics of diversified precipitation and "multiscale precipitation."…”
Section: Introductionmentioning
confidence: 99%