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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">Metaphysics</journal-id><journal-title-group><journal-title xml:lang="en">Metaphysics</journal-title><trans-title-group xml:lang="ru"><trans-title>МЕТАФИЗИКА</trans-title></trans-title-group></journal-title-group><issn publication-format="print">2224-7580</issn><publisher><publisher-name xml:lang="en">Peoples’ Friendship University of Russia named after Patrice Lumumba (RUDN University)</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">26245</article-id><article-id pub-id-type="doi">10.22363/2224-7580-2020-4-147-165</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">ANISOTROPIC GEOMETRODYNAMICS: GALACTIC TEST - STATE OF THE ART</article-title><trans-title-group xml:lang="ru"><trans-title>АНИЗОТРОПНАЯ ГЕОМЕТРОДИНАМИКА: ГАЛАКТИЧЕСКИЙ ТЕСТ - СОСТОЯНИЕ ВОПРОСА</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Siparov</surname><given-names>S. V</given-names></name><name xml:lang="ru"><surname>Сипаров</surname><given-names>Сергей Викторович</given-names></name></name-alternatives><bio xml:lang="ru">доктор физико-математических наук, профессор</bio><email>sergey@siparov.ru</email><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">State University of Civil Aviation</institution></aff><aff><institution xml:lang="ru">Государственный университет гражданской авиации</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2020-12-15" publication-format="electronic"><day>15</day><month>12</month><year>2020</year></pub-date><issue>4</issue><issue-title xml:lang="en">NO4 (2020)</issue-title><issue-title xml:lang="ru">№4 (2020)</issue-title><fpage>147</fpage><lpage>165</lpage><history><date date-type="received" iso-8601-date="2021-04-02"><day>02</day><month>04</month><year>2021</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2023, Metaphysics</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2023, МЕТАФИЗИКА</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="en">Metaphysics</copyright-holder><copyright-holder xml:lang="ru">МЕТАФИЗИКА</copyright-holder><ali:free_to_read xmlns:ali="http://www.niso.org/schemas/ali/1.0/"/></permissions><self-uri xlink:href="https://hlrsjournal.ru/metaphysics/article/view/26245">https://hlrsjournal.ru/metaphysics/article/view/26245</self-uri><abstract xml:lang="en">Anisotropic geometrodynamics contains all the known results of the general relativity theory. It also makes it possible to interpret a number of observations of the last decades without introducing new entities, but due to a change in the mathematical apparatus, and predicts the observed effects, that have not yet been interpreted. To further test the theory, an experiment is proposed, for which a theory is developed and basic observations are made. An analysis of the data obtained in the course of monitoring observations of 49 astrophysical masers (22 GHz) is presented. It is shown that the results obtained are not a consequence of instrumental errors, geophysical conditions, fluctuations in the interstellar medium, or local conditions in the vicinity of the maser. The interpretation of the observed effect is based on the phenomenon of optical-metric parametric resonance created by the action of gravitational radiation from distant short-period binaries. The stellar systems that satisfy the given conditions are revealed.</abstract><trans-abstract xml:lang="ru">Анизотропная геометродинамика содержит в себе все известные результаты общей теории относительности, позволяет интерпретировать ряд наблюдений последних десятилетий без введения новых сущностей, но за счет изменения математического аппарата и предсказывает наблюдаемые эффекты, пока не имеющие интерпретации. Для дальнейшей проверки теории предложен эксперимент, для которого разработана теория и проведены базовые наблюдения. Приводится анализ данных, полученных в ходе мониторинговых наблюдений 49 астрофизических мазеров (22 ГГц). Показано, что полученные результаты не являются следствием инструментальных ошибок, геофизических условий, флуктуаций межзвездной среды или локальных условий в окрестности мазера. Интерпретация наблюдаемого эффекта основана на явлении оптико-метрического параметрического резонанса, создаваемого воздействием гравитационного излучения удаленных короткопериодических двойных звезд. Выявлены звездные системы, удовлетворяющие заданным условиям.</trans-abstract><kwd-group xml:lang="en"><kwd>general theory of relativity</kwd><kwd>rotation curves of spiral galaxies</kwd><kwd>dark matter</kwd><kwd>generalized equivalence principle</kwd><kwd>anisotropic geometrodynamics</kwd><kwd>optical-metric parametric resonance</kwd><kwd>close binary stars</kwd><kwd>observation of periodic gravitational waves</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>общая теория относительности</kwd><kwd>кривые вращения спиральных галак- тик</kwd><kwd>темная материя</kwd><kwd>обобщенный принцип эквивалентности</kwd><kwd>анизотропная геометродинамика</kwd><kwd>оптико-метрический параметрический резонанс</kwd><kwd>тесные двойные звезды</kwd><kwd>наблюдение периодических гравитационных волн</kwd></kwd-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>Сипаров С.В. 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