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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-1619</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>АННОТАЦИИ АНГЛОЯЗЫЧНЫХ СТАТЕЙ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>ABSTRACTS ENGLISH-LANGUAGE ARTICLES</subject></subj-group></article-categories><title-group><article-title>Спектроскопические свойства наночастиц феррита марганца, допированного редкоземельным элементом Yb3+</article-title><trans-title-group xml:lang="en"><trans-title>Influence of Rare Earth Yb3+ Dopant on the Spectroscopic Properties of Manganese Ferrite Nanoparticles</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>Gulati</surname><given-names>S.</given-names></name><name name-style="western" xml:lang="en"><surname>Gulati</surname><given-names>S.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Дели</p></bio><bio xml:lang="en"><p>Sudha Gulati, Department of Physics</p><p>Delhi</p></bio><email xlink:type="simple">sudhagulati@kalindi.du.ac.in</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>Dhingra</surname><given-names>M.</given-names></name><name name-style="western" xml:lang="en"><surname>Dhingra</surname><given-names>M.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Дели</p></bio><bio xml:lang="en"><p>Mansi Dhingra, Department of Physics</p><p>Delhi</p></bio><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Колледж Калинди Делийского университета</institution></aff><aff xml:lang="en"><institution>Kalindi College, University of Delhi</institution></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Колледж Майтрейи Делийского университета</institution></aff><aff xml:lang="en"><institution>Maitreyi College, University of Delhi</institution></aff></aff-alternatives><pub-date pub-type="collection"><year>2024</year></pub-date><pub-date pub-type="epub"><day>02</day><month>08</month><year>2024</year></pub-date><volume>91</volume><issue>4</issue><fpage>606</fpage><lpage>606</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Gulati S., Dhingra M., 2024</copyright-statement><copyright-year>2024</copyright-year><copyright-holder xml:lang="ru">Gulati S., Dhingra M.</copyright-holder><copyright-holder xml:lang="en">Gulati S., Dhingra M.</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/1619">https://zhps.ejournal.by/jour/article/view/1619</self-uri><abstract><p>Методом соосаждения синтезированы наночастицы порошка MnFe2–xYbxO4 (x = 0, 0.025, 0.075, 0.1 и 0.2) различных размеров. Влияние легирующей добавки Yb3+ на свойства феррита марганца охарактеризовано методами рентгеновской дифракции (XRD), ИК-Фурье-спектроскопии (FT-IR), КР-спектроскопии и фотолюминесцентной (ФЛ) спектроскопии. Образцы имеют кубическую структуру с пространственной группой симметрии Fd3m, размеры 24.8–34.7 нм и плотность 5.07– 5.49 г/см3. ИК-Фурье-анализ указывает на наличие двух полос поглощения в диапазоне 400–600 см–1, которые характерны для ферритов. Полоса v2 (мода растяжения Fe-O в октаэдрической позиции) смещается в сторону меньшего волнового числа, что подтверждает заселенность октаэдрической позиции более крупными ионами Yb3+. Пики КР наблюдались при 228, 295, 405, 502 и 634 см–1 для нелегированного феррита марганца. В соответствии с КР-спектрами ионы Mn2+ занимают октаэдрические (B) позиции, замещая ионы Fe3+. Обнаружено, что редкоземельные ионы преимущественно занимают октаэдрические позиции. Смещение КР-полос преимущественно связано с большими радиусами редкоземельных ионов по сравнению с ионами Fe3+ и Mn2+, а смещение пиков указывает на присутствие Yb3+ в октаэдрической позиции. В спектре ФЛ наблюдается излучение при 560 нм с ростом интенсивности при увеличении содержания примеси Yb3+, что может быть связано с включением Yb3+ в структуру шпинели, приводящим к излучательной рекомбинации в желтой области электромагнитного спектра.</p></abstract><trans-abstract xml:lang="en"><p>A series of MnFe2–xYbxO4 powder nanoparticles (for x = 0, 0.025, 0.075, 0.1, and 0.2) of different crystallite sizes were synthesised using the co-precipitation method. The effect of Yb3+ dopant on the properties of manganese ferrite was characterised by X-ray diffraction (XRD), Fourier transform infrared spectroscopy (FT-IR), Raman measurements, and photoluminescence spectroscopy (PL). The crystallite size and density of the samples have a cubic structure with an Fd3m space group. Their sizes and densities were found to be in the range of 24.8–34.7 nm and 5.07–5.49 g/cc3. FT-IR analysis indicates the presence of two absorption bands in the range 400–600 cm–1, which is a fingerprint region of ferrites. The v2 band (Fe-O stretching mode of the octahedral site) shifts towards the lower wavenumber, which confirms the occupancy of larger-size Yb3+ ions at the octahedral site. The Raman peaks were observed at 228, 295, 405, 502, and 634 cm–1 for undoped manganese ferrite. Based on Raman observations, it has been observed that Mn2+ ions exhibit a preference for occupying octahedral (B) sites by substituting Fe3+ ions. Additionally, rare earth ions have been preferentially observed to occupy octahedral sites. The primary cause for the displacement of Raman bands was ascribed predominantly to the greater radii of rare earth ions in comparison to Fe3+ and Mn2+ ions, and the shifting of the peaks indicates the presence of Yb3+ at the octahedral site. The PL spectrum shows emission at 560 nm with a rise in intensity with an increase in dopant Yb3+, which could be because of the incorporation of Yb3+ in the spinel structure, leading to radiative recombination in the yellow region of the electromagnetic spectrum.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>феррит марганца</kwd><kwd>редкоземельный элемент</kwd><kwd>иттербий</kwd><kwd>ИК-Фурье-спектроскопия</kwd><kwd>комбинационное рассеяние света</kwd><kwd>фотолюминесценция</kwd></kwd-group><kwd-group xml:lang="en"><kwd>manganese ferrite</kwd><kwd>rare earth</kwd><kwd>Yb</kwd><kwd>Fourier transform infrared spectroscopy</kwd><kwd>Raman</kwd><kwd>photoluminescence</kwd></kwd-group><funding-group><funding-statement xml:lang="en">The authors would like to thank CEF, Delhi University, Delhi for the XRD measurements. 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