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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="ru"><front><journal-meta><journal-id journal-id-type="publisher-id">kaz29</journal-id><journal-title-group><journal-title xml:lang="ru">Вестник Казахстанско-Британского технического университета</journal-title><trans-title-group xml:lang="en"><trans-title>Herald of the Kazakh-British Technical University</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1998-6688</issn><issn pub-type="epub">2959-8109</issn><publisher><publisher-name>Казахстанско-Британский Технический Университет</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.55452/1998-6688-2025-22-2-322-332</article-id><article-id custom-type="elpub" pub-id-type="custom">kaz29-2016</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="ru"><subject>ФИЗИЧЕСКИЕ НАУКИ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>PHYSICAL SCIENCES</subject></subj-group></article-categories><title-group><article-title>О ТЕХНОЛОГИИ СИНТЕЗА ГИДРОГЕНИЗИРОВАННЫХ АЛМАЗОПОДОБНЫХ ТОНКИХ ПЛЕНОК ИОННО-ПЛАЗМЕННЫМ МЕТОДОМ</article-title><trans-title-group xml:lang="en"><trans-title>ON THE TECHNOLOGY OF SYNTHESIS OF HYDROGENATED DIAMOND-LIKE THIN FILMS BY ION-PLASMA METHOD</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-6255-7299</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Рягузов</surname><given-names>А. П.</given-names></name><name name-style="western" xml:lang="en"><surname>Ryaguzov</surname><given-names>A. P.</given-names></name></name-alternatives><bio xml:lang="ru"><p> к.ф.-м.н., главный научный сотрудник </p><p> г. Алматы </p></bio><bio xml:lang="en"><p> Cand. Phys.-Math. Sc., Chief Researcher </p><p> Almaty </p></bio><email xlink:type="simple">ryaguzov_a@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-4033-5492</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Әсембаева</surname><given-names>Ә. Р.</given-names></name><name name-style="western" xml:lang="en"><surname>Assembayeva</surname><given-names>A. R.</given-names></name></name-alternatives><bio xml:lang="ru"><p> PhD, ст. преподаватель </p><p> г. Алматы </p></bio><bio xml:lang="en"><p> PhD, Senior Lecturer </p><p> Almaty </p></bio><email xlink:type="simple">a.assembayeva@satbayev.university</email><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0003-4804-5323</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Гусейнов</surname><given-names>Н. Г.</given-names></name><name name-style="western" xml:lang="en"><surname>Guseinov</surname><given-names>N. R.</given-names></name></name-alternatives><bio xml:lang="ru"><p> магистр, научный сотрудник </p><p> г. Алматы </p></bio><bio xml:lang="en"><p> Master </p><p> Almaty </p></bio><email xlink:type="simple">solar_neo@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-7136-0404</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Бекмурат</surname><given-names>Ф.</given-names></name><name name-style="western" xml:lang="en"><surname>Bekmurat</surname><given-names>F.</given-names></name></name-alternatives><bio xml:lang="ru"><p> магистр физ.-техн. н., научный сотрудник </p><p> г. Алматы </p></bio><bio xml:lang="en"><p> Master </p><p> Almaty </p></bio><email xlink:type="simple">zh.fariza1@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru">ННЛОТ, Казахский национальный университет им. аль-Фараби<country>Казахстан</country></aff><aff xml:lang="en">NNLOT Al-Farabi Kazakh National University<country>Kazakhstan</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru">Казахский национальный исследовательский технический университет им. К.И. Сатпаева<country>Казахстан</country></aff><aff xml:lang="en">Satbayev University<country>Kazakhstan</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2025</year></pub-date><pub-date pub-type="epub"><day>06</day><month>07</month><year>2025</year></pub-date><volume>22</volume><issue>2</issue><fpage>322</fpage><lpage>332</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Рягузов А.П., Әсембаева Ә.Р., Гусейнов Н.Г., Бекмурат Ф., 2025</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="ru">Рягузов А.П., Әсембаева Ә.Р., Гусейнов Н.Г., Бекмурат Ф.</copyright-holder><copyright-holder xml:lang="en">Ryaguzov A.P., Assembayeva A.R., Guseinov N.R., Bekmurat F.</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://vestnik.kbtu.edu.kz/jour/article/view/2016">https://vestnik.kbtu.edu.kz/jour/article/view/2016</self-uri><abstract><p>В представленной работе рассмотрен синтез аморфных алмазоподобных углеродных пленок магнетронным методом в атмосфере смеси газов CH4+Ar. Синтез алмазоподобных пленок осуществлялся в широком диапазоне температур от 80 °С до 240 °С. Изучена локальная структура синтезированных образцов методом рамановской спектроскопии. Кроме того, изучены механические и оптические свойства полученных тонких пленок алмазоподобного углерода. Показана зависимость исследуемых характеристик от условий синтеза. Выявлено, что температура подложки существенно влияет на формирование структуры и свойства гидрогенизированных алмазоподобных углеродных пленок. Показана зависимость величины запрещенной зоны от температуры подложки. Было выявлено, что ширина запрещенной зоны синтезированных гидрогенизированных образцов уменьшается от 1,78 эВ до 1,63 эВ при увеличении температуры от 80 до 240 oC, которое можно связать с увеличением sp2 гибридизированных связей и увеличением плотности π-электронных состояний. Показано, что изменение микротвердости гидрогенизированных алмазоподобных углеродных пленок коррелирует с изменением оптической ширины запрещенной зоны. Оценка микротвердости по методу Кнупа показала, что микротвердость гидрогенизированных образцов принимает значения в интервале от 37,5×102 кгс/мм2 до 29,5×102 кгс/мм2, в зависимости от температуры подложки. Такое изменение микротвердости пленок а-С:Н подтверждает уменьшение sp3 гибридизированных связей в структуре пленок.</p></abstract><trans-abstract xml:lang="en"><p>This work presents the synthesis of hydrogenated amorphous diamond-like carbon (HDLC) films using a magnetron method in a gas mixture of CH4+Ar. The synthesis of the HDLC films was carried out over a wide temperature range from 80 °C to 240 °C. The local structure of the synthesized samples was studied using Raman spectroscopy. Additionally, the mechanical and optical properties of the obtained thin diamond-like carbon films were investigated. The dependence of the studied characteristics on the synthesis conditions was demonstrated. It was found that the substrate temperature significantly influences the formation of the structure and properties of hydrogenated diamond-like carbon films. The dependence of the bandgap on the substrate temperature was shown. It was revealed that the bandgap of the synthesized hydrogenated samples decreases from 1.78 eV to 1.63 eV as the temperature increases from 80°C to 240°C. This can be attributed to the increase in sp² hybridized bonds and the growth of π-electron density states. It was also shown that the change in microhardness of hydrogenated diamondlike carbon films correlates with the change in optical bandgap. Microhardness, evaluated using the Knoop method, was found to range from 37.5×10² kgf/mm² to 29.5×10² kgf/mm², depending on the substrate temperature. This change in microhardness confirms the decrease in sp³ hybridized bonds in the film structure.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>гидрогенизированный</kwd><kwd>алмазоподобная углеродная пленка</kwd><kwd>рамановская спектроскопия</kwd><kwd>ширина запрещенной зоны</kwd><kwd>микротвердость</kwd></kwd-group><kwd-group xml:lang="en"><kwd>hydrogenated</kwd><kwd>diamond-like carbon film</kwd><kwd>Raman spectroscopy</kwd><kwd>forbidden band width</kwd><kwd>microhardness</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Biswas H.S., Sharma R., Kumar V., et al. Nanomaterials and Energy. – 2023. – Vol. 12. – P. 160–165.</mixed-citation><mixed-citation xml:lang="en">Biswas H.S., Sharma R., Kumar V., et al. 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