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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-882</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>Уровни энергии, время жизни и радиационные данные Xe XXIV</article-title><trans-title-group xml:lang="en"><trans-title>Energy levels, lifetimes, and radiative data of Xe XXIV</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>Ren</surname><given-names>X. M.</given-names></name><name name-style="western" xml:lang="en"><surname>Ren</surname><given-names>X. M.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Наньчан, 330100</p></bio><bio xml:lang="en"><p>Nanchang, 330100</p></bio><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Hao</surname><given-names>L. H.</given-names></name><name name-style="western" xml:lang="en"><surname>Hao</surname><given-names>L. H.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Санья, Хайнань, 572022</p></bio><bio xml:lang="en"><p>Sanya, Hainan, 572022</p></bio><email xlink:type="simple">lhhao_1020@163.com</email><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Liu</surname><given-names>J. J.</given-names></name><name name-style="western" xml:lang="en"><surname>Liu</surname><given-names>J. J.</given-names></name></name-alternatives><bio xml:lang="ru"><p>Санья, Хайнань, 572022</p></bio><bio xml:lang="en"><p>Sanya, Hainan, 572022</p></bio><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Технологический институт, Институт Наньчан Цзяо Тун</institution></aff><aff xml:lang="en"><institution>Institute of Technology, Nanchang Jiao Tong Institute</institution></aff></aff-alternatives><aff-alternatives id="aff-2"><aff xml:lang="ru"><institution>Научный колледж Хайнаньского университета тропических океанов</institution></aff><aff xml:lang="en"><institution>College of Science at Hainan Tropical Ocean University</institution></aff></aff-alternatives><pub-date pub-type="collection"><year>2021</year></pub-date><pub-date pub-type="epub"><day>26</day><month>07</month><year>2021</year></pub-date><volume>88</volume><issue>4</issue><fpage>666</fpage><lpage>672</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Ren X.M., Hao L.H., Liu J.J., 2021</copyright-statement><copyright-year>2021</copyright-year><copyright-holder xml:lang="ru">Ren X.M., Hao L.H., Liu J.J.</copyright-holder><copyright-holder xml:lang="en">Ren X.M., Hao L.H., Liu J.J.</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/882">https://zhps.ejournal.by/jour/article/view/882</self-uri><abstract><p>Для расчета уровней энергии, длин волн, вероятностей переходов и сил осцилляторов для электрических дипольных разрешенных (E1) и запрещенных (M1, E2, M2) линий конфигураций 4s2 4p и 4s4p2  Xe. XXIV применен многоконфигурационный метод Дирака—Хартри-Фока. Из вероятности радиационного распада получены радиационные времена жизни 10 тонкоструктурных уровней энергии. Эффекты корреляции валентность-валентность и ядро-валентность, взаимодействия Брейта, а также эффекты квантовой электродинамики (QED) оценены в расчетах релятивистского конфигурационного взаимодействия (CI). Результаты сравниваются с экспериментальными данными и расчетами других авторов. Предсказаны новые данные для нескольких радиационных постоянных, для которых отсутствуют другие теоретические и/или экспериментальные результаты. </p></abstract><trans-abstract xml:lang="en"><p>The multi-configuration Dirac–Hartree-Fock method is employed to calculate the energy levels, wavelengths, transition probabilities, and line strengths for electric dipole allowed (E1) and forbidden (M1, E2, M2) lines for the 4s2 4p and 4s4p2  configurations of Xe XXIV. From our radiative decay probabilities, we have also derived the radiative lifetimes of 10 fine-structure energy levels. The valence–valence and core– valence correlation effects, Breit interactions, as well as quantum electrodynamics (QED) effects are estimated in the subsequent relativistic configuration interaction (CI) calculations. The present results are compared with the experimental data and with the values from other calculations. In this paper, we predict new data for several radiative data where no other theoretical and/or experimental results are available. </p></trans-abstract><kwd-group xml:lang="ru"><kwd>уровень энергии</kwd><kwd>длина волны</kwd><kwd>вероятность перехода</kwd><kwd>сила осциллятора</kwd></kwd-group><kwd-group xml:lang="en"><kwd>energy level</kwd><kwd>wavelength</kwd><kwd>transition probability</kwd><kwd>line strength</kwd></kwd-group><funding-group><funding-statement xml:lang="en">This work was supported in part by the Science and Technology Research Project of the Education Department of the Jiangxi Province of China under grant GJJ181488, the National Natural Science Foundation of China under grants 11565020, 11965010, and the Natural Science Foundation of the Hainan Province under grants 118MS071, 2019RC239.</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">J. 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