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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">10.55452/1998-6688-2024-21-3-302-313</article-id><article-id custom-type="elpub" pub-id-type="custom">kaz29-1390</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>ВЛИЯНИЕ ОТНОШЕНИЯ РАСХОДОВ ГАЗОВ N2/Ar И МОЩНОСТИ МАГНЕТРОНА НА ПЛОТНОСТЬ И СТЕХИОМЕТРИЧЕСКИЙ СОСТАВ ПЛЕНОК TINX, СИНТЕЗИРОВАННЫХ МЕТОДОМ МАГНЕТРОННОГО РАСПЫЛЕНИЯ</article-title><trans-title-group xml:lang="en"><trans-title>INFLUENCE OF THE RATIO OF GASE CONSUMPTION N2/Ar AND MAGNETRON POWER ON THE DENSITY AND STOICHIOMETRIC COMPOSITION OF TINX FILMS SYNTHESIZED BY MAGNETRON SPUTTERING 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/0000-0002-7268-7193</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Кейінбай</surname><given-names>С.</given-names></name><name name-style="western" xml:lang="en"><surname>Keiinbay</surname><given-names>S.</given-names></name></name-alternatives><bio xml:lang="ru"><p>постдокторант </p><p>050000, г. Алматы</p></bio><bio xml:lang="en"><p>postdoctoral researcher </p><p>050000, Almaty</p></bio><email xlink:type="simple">s.keiinbay@kbtu.kz</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-8200-7510</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Нусупов</surname><given-names>К. Х.</given-names></name><name name-style="western" xml:lang="en"><surname>Nussupov</surname><given-names>K. Kh.</given-names></name></name-alternatives><bio xml:lang="ru"><p>докт. физ.-матем. наук, главный научный сотрудник </p><p>050000, г. Алматы</p></bio><bio xml:lang="en"><p>Dr.Phys.-Math.Sc., chief researcher </p><p>050000, Almaty</p></bio><email xlink:type="simple">rich-famouskair@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/0000-0003-0074-431X</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Султанов</surname><given-names>А. Т.</given-names></name><name name-style="western" xml:lang="en"><surname>Sultanov</surname><given-names>A. T.</given-names></name></name-alternatives><bio xml:lang="ru"><p>докторант </p><p>050000, г. Алматы</p><p> </p></bio><bio xml:lang="en"><p>PhD student </p><p>050000, Almaty</p></bio><email xlink:type="simple">asanalisultanovs@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/0000-0002-9518-0651</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Тысченко</surname><given-names>И. Е.</given-names></name><name name-style="western" xml:lang="en"><surname>Tyschenko</surname><given-names>I. E.</given-names></name></name-alternatives><bio xml:lang="ru"><p>докт. физ.-матем. наук, ведущий научный сотрудник </p><p>630090, г. Новосибирск</p></bio><bio xml:lang="en"><p>Dr.Phys.-Math.Sc., leading researcher </p><p>630090, Novosibirsk</p></bio><email xlink:type="simple">tys@isp.nsc.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/0009-0003-4051-5180</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Эшанов</surname><given-names>А. Ф.</given-names></name><name name-style="western" xml:lang="en"><surname>Eshanov</surname><given-names>A. Ph.</given-names></name></name-alternatives><bio xml:lang="ru"><p>студент </p><p>050000, г. Алматы</p></bio><bio xml:lang="en"><p>student </p><p>050000, Almaty</p></bio><email xlink:type="simple">a_eshanov@kbtu.kz</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-5908-5614</contrib-id><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Бейсенханов</surname><given-names>Н. Б.,</given-names></name><name name-style="western" xml:lang="en"><surname>Beisenkhanov</surname><given-names>N. B.</given-names></name></name-alternatives><bio xml:lang="ru"><p>докт. физ.-матем. наук, главный научный сотрудник</p><p>050000, г. Алматы</p></bio><bio xml:lang="en"><p>Dr.Phys.-Math.Sc., chief researcher </p><p>050000, Almaty</p></bio><email xlink:type="simple">beisen@mail.ru</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru">Казахстанско-Британский технический университет<country>Казахстан</country></aff><aff xml:lang="en">Kazakh-British Technical University<country>Kazakhstan</country></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru">Институт физики полупроводников им. А.В. Ржанова Сибирского отделения Российской академии наук<country>Россия</country></aff><aff xml:lang="en">Rzhanov Institute of Semiconductor Physics, Siberian Branch of the Russian Academy of Sciences<country>Russian Federation</country></aff></aff-alternatives><pub-date pub-type="collection"><year>2024</year></pub-date><pub-date pub-type="epub"><day>03</day><month>10</month><year>2024</year></pub-date><volume>21</volume><issue>3</issue><fpage>302</fpage><lpage>313</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Кейінбай С., Нусупов К.Х., Султанов А.Т., Тысченко И.Е., Эшанов А.Ф., Бейсенханов Н.Б., 2024</copyright-statement><copyright-year>2024</copyright-year><copyright-holder xml:lang="ru">Кейінбай С., Нусупов К.Х., Султанов А.Т., Тысченко И.Е., Эшанов А.Ф., Бейсенханов Н.Б.</copyright-holder><copyright-holder xml:lang="en">Keiinbay S., Nussupov K.K., Sultanov A.T., Tyschenko I.E., Eshanov A.P., Beisenkhanov N.B.</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/1390">https://vestnik.kbtu.edu.kz/jour/article/view/1390</self-uri><abstract><p>Пленки нитрида титана были осаждены методом магнетронного распыления на постоянном токе на поверхности образцов монокристаллического кремния в атмосфере Ar-N2  для использования в качестве диффузионного барьера. Толщину и плотность пленок измеряли методом рентгеновской рефлектометрии. Изменена конструкция установки MAGNA TM-200-01 для увеличения подачи азота в камеру. Изучено влияние условий распыления, включая расход газов азота и аргона и их отношения N2 /Ar в пределах 1–60 в камере, мощность магнетрона 690 – 1400 Вт на формирование пленок TiNх , их плотность и стехиометрический состав. Показано, что на величину х влияет не только отношение расходов газов N2 /Ar, но и мощность магнетрона. При параметрах распыления 1200 Вт, N2 /Ar = 30, 0.8 Пa, 320 сек и 100 °С получена максимальная плотность 5.247 г/см3 пленки состава TiN0.786 = Ti56N44. Методом фотографической рентгеновской дифракции подтверждено наличие нанокристаллической пленки нитрида титана и отсутствие нанокристаллической фазы титана. Выявлено, что для синтеза нитрида титана, максимально близкого к стехиометрическому составу TiN0.770 – TiN0.786, необходимо использовать мощности магнетрона в пределах 900–1200 Вт, расход азота – 30 см3 /мин. при низких потоках аргона 1–5 см3 /мин.</p></abstract><trans-abstract xml:lang="en"><p>The films of titanium nitride were deposited by direct current magnetron sputtering on the surface of singlecrystalline silicon samples in an Ar-N2  atmosphere for use as a diffusion barrier. The thickness and density of films were measured by X-ray reflectometry. The design of the MAGNA TM-200-01 installation has been changed to increase the supply of nitrogen into the chamber. The influences of sputtering conditions, including the flow rate of nitrogen and argon gases and their N2 /Ar ratios in the range of 1–60 in the chamber, magnetron power of 690–1400 W on the formation of TiNx  films, their density and stoichiometric composition, were studied. It is shown that the value of x is affected not only by the N2 /Ar gas flow rate ratio, but also by the magnetron power. At the sputtering parameters 1200 W, N2 /Ar = 30, 0.8 Pa, 320 s and 100°C, a maximum density of 5.247 g/cm3  of a film was achieved, which corresponds to the composition TiN0.786 = Ti56N44. The presence of nanocrystalline film of titanium nitride and the absence of a nanocrystalline titanium phase were confirmed by photographic X-ray diffraction. It was found that for the synthesis of titanium nitride as close as possible to the stoichiometric composition TiN0.770 - TiN0.786, it is necessary to use magnetron power in the range of 900–1200 W, nitrogen rate of 30 cm3 /min with low argon flows of 1–5 cm3 /min.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>тонкие пленки</kwd><kwd>диффузионный барьер</kwd><kwd>нитрид титана</kwd><kwd>магнетронное распыление</kwd><kwd>структура</kwd></kwd-group><kwd-group xml:lang="en"><kwd>thin films</kwd><kwd>diffusion barrier</kwd><kwd>titanium nitride</kwd><kwd>magnetron sputtering</kwd><kwd>structure</kwd></kwd-group><funding-group xml:lang="ru"><funding-statement>Работа финансировалась МНВО РК в рамках проекта № AP22684659.</funding-statement></funding-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Petrov I., Hultman L., Helmersson U., Sundgren J.E., Greene J.E. 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