<article 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" article-type="research-article" dtd-version="1.2" xml:lang="ru"><front><journal-meta><journal-id journal-id-type="publisher-id">Journal of Experimental and Theoretical Physics</journal-id><journal-title-group><journal-title>Journal of Experimental and Theoretical Physics</journal-title></journal-title-group><issn publication-format="print">0044-4510</issn><issn publication-format="electronic">3034-641X</issn><publisher><publisher-name>Russian Academy of Science</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.31857/S0044451023120088</article-id><title-group><article-title>Improved Cosmological Bounds for Mixing Scenarios of Three Sterile Neutrino Generations</article-title><trans-title-group xml:lang="ru"><trans-title>Улучшенные космологические ограничения для сценариев смешивания трех поколений стерильных нейтрино</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><contrib-id contrib-id-type="orcid"></contrib-id><name-alternatives><name xml:lang="en"><surname>Dubinin</surname><given-names>M. N.</given-names></name><name xml:lang="ru"><surname>Дубинин</surname><given-names>М. Н. </given-names></name></name-alternatives><email>dubinin_m_n_noemail@ras.ru</email><xref ref-type="aff" rid="aff-1"></xref><xref ref-type="aff" rid="aff-2"></xref></contrib><contrib contrib-type="author"><contrib-id contrib-id-type="orcid"></contrib-id><name-alternatives><name xml:lang="en"><surname>Kazarkin</surname><given-names>D. M.</given-names></name><name xml:lang="ru"><surname>Казаркин</surname><given-names>Д. М. </given-names></name></name-alternatives><email>kazarkin_d_m_noemail@ras.ru</email><xref ref-type="aff" rid="aff-3"></xref></contrib></contrib-group><aff-alternatives id="aff-1"><aff><institution xml:lang="ru">Московский государственный университет им. М. В. Ломоносова</institution><institution xml:lang="en">Faculty of Physics, Moscow State University</institution></aff></aff-alternatives><aff-alternatives id="aff-2"><aff><institution xml:lang="ru"></institution><institution xml:lang="en"></institution></aff></aff-alternatives><aff-alternatives id="aff-3"><aff><institution xml:lang="ru">Московский государственный университет имени М. В. Ломоносова</institution><institution xml:lang="en">Faculty of Physics, Moscow State University</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2023-12-01" publication-format="electronic"><day>01</day><month>12</month><year>2023</year></pub-date><volume>164</volume><issue>6</issue><fpage>942</fpage><lpage>954</lpage><abstract xml:lang="en"><p>The gauge SU(2)L × U(1) model with the extension of the lepton sector by three right-handed Majorana sterile neutrinos is considered. The complete mass matrix of 6 × 6 active and sterile neutrinos is diagonalized. The cosmological bounds following from the lifetime of sterile neutrinos and the fraction of energy carried by sterile neutrino dark matter are obtained. The deviations from the “fine-tuned” mixing scenario sensitive to the mass of the lightest standard (active) neutrino are considered, and the regions of the model parameter space corresponding to these deviations are distinguished.</p></abstract><trans-abstract xml:lang="ru"><p>Рассматривается калибровочная SU (2)L × U (1) модель с расширением лептонного сектора тремя правыми майорановскими стерильными нейтрино. Проведена диагонализация полной массовой матрицы 6 × 6 активных и стерильных нейтрино. Получены космологические ограничения, вытекающие из времени жизни стерильных нейтрино и доли энергии, переносимой стерильной нейтринной темной материей. Рассмотрены отклонения от сценария «тонкой настройки» смешивания, чувствительного к массе наиболее легкого стандартного (активного) нейтрино и выделены соответствующие этим отклонениям области пространства параметров модели.</p></trans-abstract></article-meta></front><body></body><back><ref-list><ref id="B1"><label>B1</label><citation-alternatives><mixed-citation xml:lang="ru">G. Bellini, L. Ludhova, G. Ranucci, and F. Villante, Neutrino Oscillations, Adv. High Energy Phys. 2014, 191960 (2014), arXiv:1310.7858.</mixed-citation><mixed-citation xml:lang="en"></mixed-citation></citation-alternatives></ref><ref id="B2"><label>B2</label><citation-alternatives><mixed-citation xml:lang="ru">P.A. Zyla et al., Particle Data Group, Prog. Theor. Exp. Phys., 083C01, 2020.</mixed-citation><mixed-citation xml:lang="en"></mixed-citation></citation-alternatives></ref><ref id="B3"><label>B3</label><citation-alternatives><mixed-citation xml:lang="ru">R. N. Mohapatra and G. 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