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<article article-type="research-article" dtd-version="1.3" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">najo</journal-id><journal-title-group><journal-title xml:lang="en">Nanosystems: Physics, Chemistry, Mathematics</journal-title><trans-title-group xml:lang="ru"><trans-title>Наносистемы: физика, химия, математика</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">2220-8054</issn><issn pub-type="epub">2305-7971</issn><publisher><publisher-name>Университет ИТМО</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.17586/2220-8054-2026-17-4-470-481</article-id><article-id custom-type="elpub" pub-id-type="custom">najo-1909</article-id><article-categories><subj-group subj-group-type="heading"><subject>Research Article</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>PHYSICS</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="ru"><subject>ФИЗИКА</subject></subj-group></article-categories><title-group><article-title>Carbon diffusion in α-Ti and α2-Ti3Al</article-title><trans-title-group xml:lang="ru"><trans-title>Диффузия углерода в α-Ti и α2-Ti3Al</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0009-0008-0826-4074</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Горев</surname><given-names>Н. Д.</given-names></name><name name-style="western" xml:lang="en"><surname>Gorev</surname><given-names>N. D.</given-names></name></name-alternatives><bio xml:lang="en"><p>Nikita D. Gorev </p><p>pr. Akademicheskii, 2/4, Tomsk, 634055; pr. Lenina, 36, Tomsk, 634050</p><p> </p></bio><email xlink:type="simple">nkgorev@gmail.com</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-5099-3942</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Бакулин</surname><given-names>А. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Bakulin</surname><given-names>A. V.</given-names></name></name-alternatives><bio xml:lang="en"><p>Alexander V. Bakulin </p><p>pr. Akademicheskii, 2/4, Tomsk, 634055</p></bio><email xlink:type="simple">bakulin@ispms.ru</email><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-7155-3492</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Кулькова</surname><given-names>С. Е.</given-names></name><name name-style="western" xml:lang="en"><surname>Kulkova</surname><given-names>S. E.</given-names></name></name-alternatives><bio xml:lang="en"><p>Svetlana E. Kulkova </p><p>pr. Akademicheskii, 2/4, Tomsk, 634055; pr. Lenina, 36, Tomsk, 634050</p></bio><email xlink:type="simple">kulkova@ispms.ru</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff xml:lang="en" id="aff-1"><institution>Institute of Strength Physics and Materials Science of the Siberian Branch of the Russian Academy of Sciences; &#13;
National Research Tomsk State University</institution><country>Russian Federation</country></aff><aff xml:lang="en" id="aff-2"><institution>Institute of Strength Physics and Materials Science of the Siberian Branch of the Russian Academy of Sciences</institution><country>Russian Federation</country></aff><pub-date pub-type="collection"><year>2026</year></pub-date><pub-date pub-type="epub"><day>31</day><month>08</month><year>2026</year></pub-date><volume>17</volume><issue>4</issue><fpage>470</fpage><lpage>481</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Gorev N.D., Bakulin A.V., Kulkova S.E., 2026</copyright-statement><copyright-year>2026</copyright-year><copyright-holder xml:lang="ru">Горев Н.Д., Бакулин А.В., Кулькова С.Е.</copyright-holder><copyright-holder xml:lang="en">Gorev N.D., Bakulin A.V., Kulkova S.E.</copyright-holder><license xml:lang="ru" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>Данная работа распространяется под лицензией Creative Commons Attribution 4.0.</license-p></license><license xml:lang="en" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>This work is licensed under a Creative Commons Attribution 4.0 License.</license-p></license></permissions><self-uri xlink:href="https://nanojournal.ifmo.ru/jour/article/view/1909">https://nanojournal.ifmo.ru/jour/article/view/1909</self-uri><abstract><p>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.</p></abstract><trans-abstract xml:lang="ru"><p>Методом проекционных присоединенных волн рассчитаны энергии образования дефектов внедрения углерода в различных междоузлиях, заселенности кристаллических орбиталей Гамильтона, функция локализации электронов, объемы Вороного и другие характеристики α-Ti и α2-Ti3Al. Для оценки барьеров миграции вдоль путей между стабильными позициями внедрения использовался метод подталкивающих упругих связей с восходящим изображением. Температурно-зависимые коэффициенты диффузии углерода были оценены вдоль двух неэквивалентных кристаллографических направлений (a и c) в α-Ti и, впервые, в α2-Ti3Al. Энергетически предпочтительной позицией как в α-Ti, так и в α2-Ti3Al является октаэдрическая, локальное окружение которой содержит только атомы Ti. Эта предпочтительность зависит от материала и в первую очередь обусловлена низким механическим вкладом в энергию образования дефектов в α-Ti и химическим вкладом в случае сплава. Присутствие Al приводит к увеличению энергии образования дефектов в сплаве. В случае α-Ti полученные коэффициенты диффузии хорошо согласуются с экспериментом. Присутствие алюминия в сплаве приводит к замедлению диффузии углерода из-за более высоких энергий как образования дефектов, так и миграции.</p><p> </p></trans-abstract><kwd-group xml:lang="ru"><kwd>титан</kwd><kwd>алюминид титана</kwd><kwd>диффузия углерода</kwd><kwd>первопринципные расчеты</kwd></kwd-group><kwd-group xml:lang="en"><kwd>titanium</kwd><kwd>titanium aluminide</kwd><kwd>carbon diffusion</kwd><kwd>ab-initio calculations</kwd></kwd-group><funding-group><funding-statement xml:lang="en">The work was performed according to the Government research assignment for ISPMS SB RAS, project FWRW-2026-0008. 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