Abstract

Generalized stacking fault energy (GSFE) is an important parameter for understanding the underlying physics governing the deformation mechanisms in face-centred cubic (fcc) materials. In the present work, we study the long-standing question regarding the influence of C on the GSFE in austenitic steels at paramagnetic state. We calculate the GSFE in both -Fe and Fe–C alloys using the exact muffin-tin orbitals method and the Vienna Ab initio Simulation Package. Our results show that the GSFE is increased by the presence of interstitial C, and the universal scaling law is used to verify the accuracy of the obtained stacking fault energies. The C-driven change of the GSFE is discussed considering the magnetic contributions. The effective energy barriers for stacking fault, twinning and slip formation are employed to disclose the C effect on the deformation modes, and we also demonstrate that the magnetic structures as a function of volume explain the effect of paramagnetism on the C-driven changes of the stacking fault energies as compared to the hypothetical non-magnetic case.

Highlights

  • Mechanical twinning and -martensite transformation are two primary deformation mechanisms competing with full dislocation glide in the so-called twinning-induced plasticity (TWIP) and transformation-induced plasticity (TRIP) steels

  • Our results show that the Generalized stacking fault energy (GSFE) is increased by the presence of interstitial C, and the universal scaling law is used to verify the accuracy of the obtained stacking fault energies

  • The effective energy barriers for stacking fault, twinning and slip formation are employed to disclose the C effect on the deformation modes, and we demonstrate that the magnetic structures as a function of volume explain the effect of paramagnetism on the C-driven changes of the stacking fault energies as compared to the hypothetical non-magnetic case

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Summary

Introduction

Mechanical twinning and -martensite transformation are two primary deformation mechanisms competing with full dislocation glide in the so-called twinning-induced plasticity (TWIP) and transformation-induced plasticity (TRIP) steels. These steels possess a balanced combination of strength and elongation, making them promising materials for applications in automotive industry. One central problem is related to modelling the magnetic state of austenitic steels [2], whose Curie/Néel temperatures are usually lower than room temper­ ature [3].

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