2014
DOI: 10.2478/amm-2014-0205
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Elaboration of Thermomechanical Treatment Conditions of Ti-V and Ti-Nb-V Microalloyed Forging Steels

Abstract: The goal of the work was to describe the forging conditions of thermomechanical treatment for Ti-V and Ti-Nb-V microalloyed steels. Conditions of hot-working allowing to obtain both the desired microstructure and mechanical properties of forgings were selected taking into consideration: precipitation analysis of MX-type (M-Nb, Ti, V; X-N, C) interstitial phases in austenite; research on the influence of the austenitizing temperature on the γ-phase grain size; investigation of the continuous compression of spec… Show more

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Cited by 24 publications
(18 citation statements)
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“…The precipitation hardening was mainly triggered by dispersive precipitates of several nanometres in size, precipitated in the steel (in ferrite) during cooling ( Figure 2) [28][29][30][31][32]. Particles sized above twenty nanometres did not significantly contribute to precipitation hardening, yet they restrained the recrystallised austenite grain growth, favouring the formation of the fine-grained structure [28,[33][34][35][36][37]. The recrystallised austenite grain growth in the test steel was primarily restrained by precipitates of globular (Nb,Ti)C carbides of approximately 10 nm in diameter and characterised by niobium predominance [38], precipitates of (Ti,Nb)C carbides of approximately 20 nm in size, and (Ti,Nb)(C,N) precipitates of approximately 50 nm in size.…”
Section: Resultsmentioning
confidence: 99%
“…The precipitation hardening was mainly triggered by dispersive precipitates of several nanometres in size, precipitated in the steel (in ferrite) during cooling ( Figure 2) [28][29][30][31][32]. Particles sized above twenty nanometres did not significantly contribute to precipitation hardening, yet they restrained the recrystallised austenite grain growth, favouring the formation of the fine-grained structure [28,[33][34][35][36][37]. The recrystallised austenite grain growth in the test steel was primarily restrained by precipitates of globular (Nb,Ti)C carbides of approximately 10 nm in diameter and characterised by niobium predominance [38], precipitates of (Ti,Nb)C carbides of approximately 20 nm in size, and (Ti,Nb)(C,N) precipitates of approximately 50 nm in size.…”
Section: Resultsmentioning
confidence: 99%
“…The use of advanced technologies in metallurgical processing as well as a new look at the significance and the role of alloying elements used in steels have enabled the fabrication of various groups of steels characterised by vast ranges of mechanical and plastic properties [1]. The development of new steel grades, particularly high-strength low alloys (HSLA) having ferritic, ferritic-pearlitic, ferritic-bainitic, bainitic, or tempered martensitic structures, has made it possible to significantly reduce the weight of structural elements and that of entire structures [2][3][4]. The reduction of thicknesses of steels manufactured in thermo-mechanical control processes (TMCP) (dictated by the needs of the automotive, ship-building, and petroleum industries) without compromising previously obtained performance characteristics has made it possible to achieve significant savings resulting from lower material processing and transport-related costs [5][6][7][8][9][10][11].…”
Section: Introductionmentioning
confidence: 99%
“…The selected temperature and grain size may seem to be too low. However, the aim was to take into account a grain size after plastic deformation, which is usually successfully decreased during multistep deformation tests [21,24]. The pearlite transformation starts after ca.…”
Section: Thermodynamic Calculationsmentioning
confidence: 99%
“…It should be taken into account that plastic deformation shifts diffusion-controlled transformations to a shorter time [31,32]. JMatPro software does not enable the user to take into take into account a grain size after plastic deformation, which is usually successfully decreased during multistep deformation tests [21,24]. The pearlite transformation starts after ca.…”
Section: Thermodynamic Calculationsmentioning
confidence: 99%