<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE root>
<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">Astronomy Reports</journal-id><journal-title-group><journal-title xml:lang="en">Astronomy Reports</journal-title><trans-title-group xml:lang="ru"><trans-title>Астрономический журнал</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0004-6299</issn><issn publication-format="electronic">3034-5170</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">355481</article-id><article-id pub-id-type="doi">10.7868/S3034518925110011</article-id><article-categories><subj-group subj-group-type="toc-heading" xml:lang="en"><subject>Articles</subject></subj-group><subj-group subj-group-type="toc-heading" xml:lang="ru"><subject>СТАТЬИ</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">REGISTRATION OF BURSTS OF GRAVITY-GRADIENT AND NEUTRINO BACKGROUND BY UNDERGROUND DETECTORS</article-title><trans-title-group xml:lang="ru"><trans-title>РЕГИСТРАЦИЯ ВСПЛЕСКОВ ГРАВИ-ГРАДИЕНТНОГО И НЕЙТРИННОГО ФОНА ПОДЗЕМНЫМИ ДЕТЕКТОРАМИ</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Rudenko</surname><given-names>V. N.</given-names></name><name xml:lang="ru"><surname>Руденко</surname><given-names>В. Н.</given-names></name></name-alternatives><email>valentin.rudenko@gmail.com</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Gavrilyuk</surname><given-names>Yu. M.</given-names></name><name xml:lang="ru"><surname>Гаврилюк</surname><given-names>Ю. М.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff2"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Gusev</surname><given-names>A. V.</given-names></name><name xml:lang="ru"><surname>Гусев</surname><given-names>А. В.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Oreshkin</surname><given-names>S. I.</given-names></name><name xml:lang="ru"><surname>Орешкин</surname><given-names>С. И.</given-names></name></name-alternatives><email>sioresh@yahoo.com</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Popov</surname><given-names>S. M.</given-names></name><name xml:lang="ru"><surname>Попов</surname><given-names>С. М.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Kvashnin</surname><given-names>N. L.</given-names></name><name xml:lang="ru"><surname>Квашнин</surname><given-names>Н. Л.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff3"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Lugovoy</surname><given-names>A. A.</given-names></name><name xml:lang="ru"><surname>Луговой</surname><given-names>А. А.</given-names></name></name-alternatives><xref ref-type="aff" rid="aff3"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">Sternberg State Astronomical Institute, Lomonosov Moscow State University</institution></aff><aff><institution xml:lang="ru">Астрономический институт им. П. К. Штернберга, Московский государственный университет им. М. В. Ломоносова</institution></aff></aff-alternatives><aff-alternatives id="aff2"><aff><institution xml:lang="en">Nuclear Research Institute RAS, Baksan Neutrino Observatory</institution></aff><aff><institution xml:lang="ru">Баксанская нейтринная обсерватория, Институт ядерных исследований РАН</institution></aff></aff-alternatives><aff-alternatives id="aff3"><aff><institution xml:lang="en">Laser Physics Institute SB RAS</institution></aff><aff><institution xml:lang="ru">Институт лазерной физики СО РАН</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2025-11-15" publication-format="electronic"><day>15</day><month>11</month><year>2025</year></pub-date><volume>102</volume><issue>11</issue><issue-title xml:lang="en">VOL 102, NO11 (2025)</issue-title><issue-title xml:lang="ru">ТОМ 102, №11 (2025)</issue-title><fpage>963</fpage><lpage>974</lpage><history><date date-type="received" iso-8601-date="2025-12-02"><day>02</day><month>12</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="2026-11-15"/></permissions><self-uri xlink:href="https://journals.rcsi.science/0004-6299/article/view/355481">https://journals.rcsi.science/0004-6299/article/view/355481</self-uri><abstract xml:lang="en"><p>The problem of registration of collapsing stars in the Galaxy is considered using two instruments: the optoacoustic gravitational detector OGRAN and the neutrino telescope BUST, located in the underground laboratories of the BNO INR RAS. An algorithm for joint data processing on the experience of registration of the SN1987A event is presented. The proposed method is illustrated by the current output signals of these instruments.</p></abstract><trans-abstract xml:lang="ru"><p>Рассматривается задача регистрации коллагентрующих звезд в Галактике с помощью двух инструментов: оптоакустического гравитационного детектора ОГРАН и нейтринного телескопа БПСТ, расположенных в подземных лабораториях БНО ИЯИ РАН. Представлен алгоритм совместной обработки данных по опыту регистрации события SN1987A. Предлагаемая методика иллюстрируется на текущих выходных сигналах указанных инструментов.</p></trans-abstract><kwd-group xml:lang="en"><kwd>gravitational collapse</kwd><kwd>gravitational detectors</kwd><kwd>neutrino telescopes</kwd><kwd>gravitational-neutrino correlations</kwd><kwd>multichannel astronomy</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>гравитационный коллапс</kwd><kwd>гравитационные детекторы</kwd><kwd>нейтринные телескопы</kwd><kwd>гравитационно-нейтринные корреляции</kwd><kwd>мультиканальная астрономия</kwd></kwd-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>B.P. Abbott, et al., Phys. Rev. Lett. 116, 061102 (2016).</mixed-citation></ref><ref id="B2"><label>2.</label><mixed-citation>B.P. Abbott, et al., Phys. Rev. Lett. 118, 221101 (2017).</mixed-citation></ref><ref id="B3"><label>3.</label><mixed-citation>B.P. Abbott, et al., Phys. Rev. Lett. 119, 141101 (2017).</mixed-citation></ref><ref id="B4"><label>4.</label><mixed-citation>B.P. Abbott, et al. Phys. Rev. Lett. 119, 161101 (2017).</mixed-citation></ref><ref id="B5"><label>5.</label><mixed-citation>A. von Kienlin, C. Meegan and A. Goldstein, GRB Coordinates Network, Circular Service 21520, 1 (2017).</mixed-citation></ref><ref id="B6"><label>6.</label><mixed-citation>V. Savchenko et al., Astrophys. J. 848(2), L15 (2017).</mixed-citation></ref><ref id="B7"><label>7.</label><mixed-citation>M. Punturo et al., Classical and Quantum Gravity 27(8):084007 (Apr 2010),</mixed-citation></ref><ref id="B8"><label>8.</label><mixed-citation>Astro2020 Science White Paper. Gravitational wave astronomy with LIGO and similar detectors in the next decade. arXiv:1904.03187v1 [gr-qc] 5 Apr 2019.</mixed-citation></ref><ref id="B9"><label>9.</label><mixed-citation>R.X. Adhikari, Rev. Mod. Phys. 86, 121 (Feb 2014),</mixed-citation></ref><ref id="B10"><label>10.</label><mixed-citation>Y. Novoseltsev, M. Boliev, V. Volchenko, et al, J. Exp. Theor. Phys. 125(1), 73–79 (2017).</mixed-citation></ref><ref id="B11"><label>11.</label><mixed-citation>Y. Novoseltsev, I. Dzaparova, Kochkarov, et al., Neutrino Burst Monitoring in Our Galaxy. J. Exp. Theor. Phys. 134, 390–398 (2022).</mixed-citation></ref><ref id="B12"><label>12.</label><mixed-citation>W. Baade, F. Zwicky, Proceedings of the National Academy of Science 20, 254 (1934),</mixed-citation></ref><ref id="B13"><label>13.</label><mixed-citation>G.S. Bisnovatyi-Kogan, V.S. Imshennik, D.K. Nadyozin et al. Astrophysics and Space Science 35, 23–41 (1975).</mixed-citation></ref><ref id="B14"><label>14.</label><mixed-citation>M.B. Пружинская Сверхновые звезды, гамма-велигерка и ускорение расширение Вселенной (sai. msu.ru &gt; dissovet/prizhinskaya_thesis.pdf).</mixed-citation></ref><ref id="B15"><label>15.</label><mixed-citation>V.N. Rudenko, Yu.M. Gavrilyuk, A.V. Gusev, et al, International Journal of Modern Physics A 35, Nos. 2 &amp; 3, 2040007 (2020).</mixed-citation></ref><ref id="B16"><label>16.</label><mixed-citation>S.N. Bagaev, L.B. Bezrukov, N.L. Kvashnin, V.A. Krysanov, S.I. Oreshkin, A.M. Motylev, S.M. Popov, V.N. Rudenko, A.A. Samoilenko, M.N. Skvortsov, et al. Rev. Sci. Instrum. 85, 065114 (2014).</mixed-citation></ref><ref id="B17"><label>17.</label><mixed-citation>V.N. Rudenko, Physics–Uspekhi 60, 830–842 (2017).</mixed-citation></ref><ref id="B18"><label>18.</label><mixed-citation>V. Rudenko, N. Kvashnin, A. Lugovoi, S. Oreshkin, S. Popov, A. Samoylenko, M. Skvortsov, I. Yudin, Setup. Phys. At. Nucl. 83, 1682–1690 (2020).</mixed-citation></ref><ref id="B19"><label>19.</label><mixed-citation>V.N. Rudenko, V.A. Silin, A.N. Tsepkov, Astronomy Reports 56, № 8, 638–652 (2012).</mixed-citation></ref><ref id="B20"><label>20.</label><mixed-citation>B.H. Руденко, A.B. Гусев, A.B. Сердобольский, Г. Пиццелла, Измерительная техника № 10, 3–7 (2004).</mixed-citation></ref><ref id="B21"><label>21.</label><mixed-citation>S. Andrusenko, Y. Gavriluk, A. Gusev et al., Universe 8(9), 446 (2022).</mixed-citation></ref><ref id="B22"><label>22.</label><mixed-citation>H.H. Чугай Земля и Вселенная (M., Наука, № 2, 22–30, 1989).</mixed-citation></ref><ref id="B23"><label>23.</label><mixed-citation>E. Amaldi et al., Europhys. Lett. 3 1325 (1987).</mixed-citation></ref><ref id="B24"><label>24.</label><mixed-citation>M. Aglietta, A. Castellina, W. Fulgione et al., Nuovo Cimento C 14, 171 (1991).</mixed-citation></ref><ref id="B25"><label>25.</label><mixed-citation>C.A. Dickson, B.F. Schutz, Phys. Rev. D 51 2644 (1995).</mixed-citation></ref><ref id="B26"><label>26.</label><mixed-citation>V.N. Rudenko, A.V. Gusev, V.K. Kravchuk et al., JETP 91, № 5, 845–858 (2000).</mixed-citation></ref><ref id="B27"><label>27.</label><mixed-citation>Ю.Н. Ерошенко, Е.О. Бабичев, В.И. Докучаев et al., ЖЭТФ 155, № 4, 702–710 (2019).</mixed-citation></ref></ref-list></back></article>
