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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">zhps</journal-id><journal-title-group><journal-title xml:lang="ru">Журнал прикладной спектроскопии</journal-title><trans-title-group xml:lang="en"><trans-title>Zhurnal Prikladnoii Spektroskopii</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">0514-7506</issn><publisher><publisher-name>B. I. Stepanov Institute of Physics of the National Academy of Sciences</publisher-name></publisher></journal-meta><article-meta><article-id custom-type="elpub" pub-id-type="custom">zhps-1360</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>ОПТИЧЕСКИЕ МАТЕРИАЛЫ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>OPTICAL MATERIALS</subject></subj-group></article-categories><title-group><article-title>Структурные и фотоэлектрические свойства перовскитных солнечных элементов из CsPbI3, изготовленных с добавлением иодистоводородной кислоты</article-title><trans-title-group xml:lang="en"><trans-title>Structural and Photoelectric Properties of CsPbI3 Perovskite Solar Elements Made with Hydriodic Acid Adding</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Захидов</surname><given-names>Э. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Zakhidov</surname><given-names>E. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ташкент</p></bio><email xlink:type="simple">ezakhidov@hotmail.com</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Нематов</surname><given-names>Ш. К.</given-names></name><name name-style="western" xml:lang="en"><surname>Nematov</surname><given-names>Sh. K.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ташкент</p></bio><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Сапарбаев</surname><given-names>А. А.</given-names></name><name name-style="western" xml:lang="en"><surname>Saparbaev</surname><given-names>A. A.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ташкент</p></bio><email xlink:type="simple">saparbaevaziz83@gmail.com</email><xref ref-type="aff" rid="aff-3"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Нурумбетова</surname><given-names>Л. Р.</given-names></name><name name-style="western" xml:lang="en"><surname>Nurumbetova</surname><given-names>L. R.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ташкент</p></bio><xref ref-type="aff" rid="aff-4"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Хидиров</surname><given-names>Б. Г.</given-names></name><name name-style="western" xml:lang="en"><surname>Khidirov</surname><given-names>B. G.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ташкент</p></bio><xref ref-type="aff" rid="aff-4"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Тургунбоев</surname><given-names>А. Ю.</given-names></name><name name-style="western" xml:lang="en"><surname>Turgunboev</surname><given-names>A. Yu.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Ташкент</p></bio><xref ref-type="aff" rid="aff-4"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт ионно-плазменных и лазерных технологий АН РУз</institution></aff><aff xml:lang="en"><institution>Institute of Ion-Plasma and Laser Technologies of Academy of Sciences of the Republic of Uzbekistan</institution></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Национальный университет Узбекистана имени Мирзо Улугбека</institution></aff><aff xml:lang="en"><institution>Mirzo Ulugbek National University of Uzbekistan</institution></aff></aff-alternatives><aff-alternatives id="aff-3"><aff xml:lang="ru"><institution>Институт ионно-плазменных и лазерных технологий АН РУз;&#13;
Национальный университет Узбекистана имени Мирзо Улугбека;&#13;
Ташкентский государственный технический университет имени Ислама Каримова</institution></aff><aff xml:lang="en"><institution>Institute of Ion-Plasma and Laser Technologies of Academy of Sciences of the Republic of Uzbekistan;&#13;
Mirzo Ulugbek National University of Uzbekistan;&#13;
Islam Karimov Tashkent State Technical University</institution></aff></aff-alternatives><aff-alternatives id="aff-4"><aff xml:lang="ru"><institution>Институт ионно-плазменных и лазерных технологий АН РУз;&#13;
Ташкентский государственный технический университет имени Ислама Каримова</institution></aff><aff xml:lang="en"><institution>Institute of Ion-Plasma and Laser Technologies of Academy of Sciences of the Republic of Uzbekistan;&#13;
Islam Karimov Tashkent State Technical University</institution></aff></aff-alternatives><pub-date pub-type="collection"><year>2023</year></pub-date><pub-date pub-type="epub"><day>25</day><month>08</month><year>2023</year></pub-date><volume>90</volume><issue>4</issue><fpage>640</fpage><lpage>647</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Захидов Э.А., Нематов Ш.К., Сапарбаев А.А., Нурумбетова Л.Р., Хидиров Б.Г., Тургунбоев А.Ю., 2023</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="ru">Захидов Э.А., Нематов Ш.К., Сапарбаев А.А., Нурумбетова Л.Р., Хидиров Б.Г., Тургунбоев А.Ю.</copyright-holder><copyright-holder xml:lang="en">Zakhidov E.A., Nematov S.K., Saparbaev A.A., Nurumbetova L.R., Khidirov B.G., Turgunboev A.Y.</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://zhps.ejournal.by/jour/article/view/1360">https://zhps.ejournal.by/jour/article/view/1360</self-uri><abstract><p>Неорганические перовскиты на основе трииодида цезия-свинца (CsPbI3) остаются наиболее перспективным материалом для изготовления перовскитных солнечных элементов (ПСЭ) за счет оптимальной ширины запрещенной зоны ~1.72 эВ и высокого коэффициента поглощения света. Последнее характерно для кубической структуры CsPbI3, так называемой черной фазы. Для образования такой структуры при относительно низких температурах требуется добавление иодистоводородной кислоты (HI) в раствор перовскита, из которого она готовится. Изучены структурные, морфологические, оптические и фотоэлектрические параметры солнечных элементов CsPbI3 при различных концентрациях (добавленном количестве) кислоты HI. Описаны важнейшие характеристики ПСЭ из CsPbI3 с максимальной эффективностью 8.85 %, полученные при концентрации HI-кислоты 66 мкл/мл.</p></abstract><trans-abstract xml:lang="en"><p>Caesium-lead-triiodide (CsPbI3) – based inorganic perovskites are the most perspective material for production of perovskite solar cells (PSC) due to the optimal width of energy gap in them, about 1.72 eV and high light absorption coefficient. The latter is the characteristic of the cubic structure of CsPbI3, called the black phase. To form such a structure at relatively low temperatures, it is required to add hydroiodic acid (HI) to the perovskite solution from which the structure is prepared. Structural, morphological, optical and photoelectrical parameters of CsPbI3 solar cells at various concentrations (added quantity) of HI acid have been studied. The most important characteristics of CsPbI3 – based PSC with maximum efficiency of 8.85% obtained at HI acid concentration of 66 µl/ml are described.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>перовскит</kwd><kwd>иодид свинца</kwd><kwd>солнечные элементы</kwd><kwd>иодистоводородная кислота</kwd></kwd-group><kwd-group xml:lang="en"><kwd>perovskite</kwd><kwd>lead iodide</kwd><kwd>solar elements</kwd><kwd>HI acide</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Работа выполнена в рамках программы фундаментальных исследований (проект ФЗ-20200929177).</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">Wang, K. Li, R. Wang, Z.-K. Wang, M. Li, Y. Zhang, H. Ma, L.-S. Liao, Y. Yang. Nano Lett., 19, N 8 (2019) 5176—5184</mixed-citation><mixed-citation xml:lang="en">Wang, K. Li, R. Wang, Z.-K. Wang, M. Li, Y. Zhang, H. Ma, L.-S. Liao, Y. 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