Carbon diffusion in α-Ti and α2-Ti3Al
https://doi.org/10.17586/2220-8054-2026-17-4-470-481
Abstract
The interstitial defect formation energies of carbon in various interstices, crystal orbital Hamilton populations, electron localization function, Voronoi volumes, and other characteristics in α-Ti and α2-Ti3Al were calculated by the projector augmented wave method. The climbing image nudged elastic band method was used to estimate migration barriers along paths between stable interstitials. The temperature-dependent diffusion coefficients of carbon were evaluated along two nonequivalent crystallographic directions (a and c) in α-Ti and, for the first time, in α2-Ti3Al. The energetically preferred site in both α-Ti and α2-Ti3Al is an octahedral one, whose local environment contains only Ti atoms. This preference depends on material and is primarily due to low mechanical contribution to the defect formation energy in α-Ti and chemical one in the case of the alloy. The presence of Al leads to an increase in the defect formation energy in the alloy. In the case of α-Ti, the obtained diffusion coefficients are in good agreement with experiment. Aluminum in the alloy leads to a slowdown in carbon diffusion due to higher both defect formation and migration energies.
About the Authors
N. D. GorevRussian Federation
Nikita D. Gorev
pr. Akademicheskii, 2/4, Tomsk, 634055;
pr. Lenina, 36, Tomsk, 634050
A. V. Bakulin
Russian Federation
Alexander V. Bakulin
pr. Akademicheskii, 2/4, Tomsk, 634055
S. E. Kulkova
Russian Federation
Svetlana E. Kulkova
pr. Akademicheskii, 2/4, Tomsk, 634055;
pr. Lenina, 36, Tomsk, 634050
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Review
For citations:
Gorev N.D., Bakulin A.V., Kulkova S.E. Carbon diffusion in α-Ti and α2-Ti3Al. Nanosystems: Physics, Chemistry, Mathematics. 2026;17(4):470-481. https://doi.org/10.17586/2220-8054-2026-17-4-470-481
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