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<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" xmlns:ali="http://www.niso.org/schemas/ali/1.0/" article-type="research-article" dtd-version="1.2" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">Physics of Atomic Nuclei</journal-id><journal-title-group><journal-title xml:lang="en">Physics of Atomic Nuclei</journal-title><trans-title-group xml:lang="ru"><trans-title>Ядерная физика</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0044-0027</issn><issn publication-format="electronic">3034-6282</issn><publisher><publisher-name xml:lang="en">The Russian Academy of Sciences</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">696597</article-id><article-id pub-id-type="doi">10.31857/S0044002725040042</article-id><article-categories><subj-group subj-group-type="toc-heading"><subject>ЭЛЕМЕНТАРНЫЕ ЧАСТИЦЫ И ПОЛЯ. Эксперимент</subject></subj-group><subj-group subj-group-type="article-type"><subject>Research Article</subject></subj-group></article-categories><title-group><article-title xml:lang="en">Study of the solar neutrino interaction with 128,130Te nuclei and the large Baksan neutrino telescope project</article-title><trans-title-group xml:lang="ru"><trans-title>ИССЛЕДОВАНИЕ ВЗАИМОДЕЙСТВИЯ СОЛНЕЧНЫХ НЕЙТРИНО С ЯДРАМИ 128,130Тe И ПРОЕКТ БОЛЬШОГО БАКСАНСКОГО НЕЙТРИННОГО ТЕЛЕСКОПА</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Lutostansky</surname><given-names>Yu. S.</given-names></name><name xml:lang="ru"><surname>Лютостанский</surname><given-names>Ю. С.</given-names></name></name-alternatives><email>lutostanskiy@yandex.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Fazliakhmetov</surname><given-names>A. N.</given-names></name><name xml:lang="ru"><surname>Фазлиахметов</surname><given-names>А. Н.</given-names></name></name-alternatives><email>fazliakhmetov@phystech.edu</email><xref ref-type="aff" rid="aff1"/><xref ref-type="aff" rid="aff2"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Lubsandorzhiev</surname><given-names>B. K.</given-names></name><name xml:lang="ru"><surname>Лубсандоржиев</surname><given-names>Б. К.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff2"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Koroteev</surname><given-names>G. A.</given-names></name><name xml:lang="ru"><surname>Коротеев</surname><given-names>Г. А.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff2"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Tikhonov</surname><given-names>V. N.</given-names></name><name xml:lang="ru"><surname>Тихонов</surname><given-names>В. Н.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">National Research Centre “Kurchatov Institute”</institution></aff><aff><institution xml:lang="ru">Национальный исследовательский центр “Курчатовский институт”</institution></aff></aff-alternatives><aff-alternatives id="aff2"><aff><institution xml:lang="en">Institute for Nuclear Research of the Russian Academy of Sciences</institution></aff><aff><institution xml:lang="ru">Институт ядерных исследований Российской академии наук</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2025-08-15" publication-format="electronic"><day>15</day><month>08</month><year>2025</year></pub-date><volume>88</volume><issue>4</issue><issue-title xml:lang="en">VOL 88, NO4 (2025)</issue-title><issue-title xml:lang="ru">ТОМ 88, №4 (2025)</issue-title><fpage>345</fpage><lpage>355</lpage><history><date date-type="received" iso-8601-date="2025-11-20"><day>20</day><month>11</month><year>2025</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2025, Russian Academy of Sciences</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2025, Российская академия наук</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="en">Russian Academy of Sciences</copyright-holder><copyright-holder xml:lang="ru">Российская академия наук</copyright-holder><ali:free_to_read xmlns:ali="http://www.niso.org/schemas/ali/1.0/" start_date="2026-08-15"/></permissions><self-uri xlink:href="https://transsyst.ru/0044-0027/article/view/696597">https://transsyst.ru/0044-0027/article/view/696597</self-uri><abstract xml:lang="en"><p>The interaction of neutrinos with tellurium nuclei 128 and 130 has been studied, taking into account the influence of charge-exchange resonances. The paper presents calculations of the cross section of solar neutrino capture σ(Eν) by the isotopes 128Te and 130Te. Both experimental data on the strength functions S(E), obtained in the charge-exchange reaction (3He, t) and the S(E) functions calculated within the framework of the microscopic theory of finite Fermi-systems were used. The influence of the resonant structure S(E) on the calculated capture cross sections of solar neutrinos was studied and the contributions of each of the high-lying resonances to the capture cross section σ(Eν) were identified. The contributions of all components of the solar neutrino spectrum were calculated. The contribution of background solar neutrinos to the double beta decay of 130Те nuclei was estimated.</p></abstract><trans-abstract xml:lang="ru"><p>Исследован процесс взаимодействия нейтрино с ядрами теллура 128 и 130 с учетом влияния зарядово-обменных резонансов. В работе представлены расчеты сечения захвата солнечных нейтрино σ(Eν) изотопами 128Те и 130Те. Использовались как экспериментальные данные по силовым функциям S(E), полученные в зарядово-обменной реакции (3He, t), так и функции S(E), рассчитанные в рамках микроскопической теории конечных Ферми-систем. Исследовалось влияние резонансной структуры S(E) на рассчитываемые сечения захвата солнечных нейтрино, и выделены вклады каждого из высоколежащих резонансов в сечение захвата σ(Eν). Рассчитаны вклады всех компонентов солнечного нейтринного спектра. Оценен вклад фоновых солнечных нейтрино в двойной бета-распад ядер 130Те.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>солнечные нейтрино</kwd><kwd>захват нейтриноядрами</kwd><kwd>изотопы теллура 128,130Тe</kwd><kwd>зарядово-обменные реакции</kwd><kwd>нейтринный телескоп</kwd></kwd-group><funding-group><funding-statement xml:lang="ru">Работа выполнена при поддержке федерального бюджета и Минобрнауки РФ в рамках программы финансирования крупных научных проектов, национального проекта «Наука», № 075-15-2024-541.</funding-statement></funding-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>J. A. Formaggio and G. P. Zeller, Rev. Mod. Phys. 84, 1307 (2012).</mixed-citation></ref><ref id="B2"><label>2.</label><mixed-citation>Дж. Бакал, Нейтринная астрофизика (Мир, Москва, 1993) [J. N. Bahcall, Neutrino Astrophysics (Cambridge Univ. Press, Cambridge, 1989)].</mixed-citation></ref><ref id="B3"><label>3.</label><mixed-citation>J. 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