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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">vestifm</journal-id><journal-title-group><journal-title xml:lang="ru">Известия Национальной академии наук Беларуси. Серия физико-математических наук</journal-title><trans-title-group xml:lang="en"><trans-title>Proceedings of the National Academy of Sciences of Belarus. Physics and Mathematics Series</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">1561-2430</issn><issn pub-type="epub">2524-2415</issn><publisher><publisher-name>The Republican Unitary Enterprise Publishing House "Belaruskaya Navuka"</publisher-name></publisher></journal-meta><article-meta><article-id custom-type="elpub" pub-id-type="custom">vestifm-276</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>ФИЗИКА</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>PHYSICS</subject></subj-group></article-categories><title-group><article-title>ИСПОЛЬЗОВАНИЕ КРИСТАЛЛОВ В ФИЗИКЕ ВЫСОКИХ ЭНЕРГИЙ ДЛЯ НАБЛЮДЕНИЯ НОВЫХ ЯВЛЕНИЙ И РАЗВИТИЯ УСКОРИТЕЛЬНЫХ ТЕХНОЛОГИЙ</article-title><trans-title-group xml:lang="en"><trans-title>CRYSTAL APPLICATIONS IN HIGH ENERGY PHYSICS FOR NEW PHENOMENA OBSERVATION AND ACCELERATION TECHNOLOGY DEVELOPMENT</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>Барышевский</surname><given-names>В. Г.</given-names></name><name name-style="western" xml:lang="en"><surname>Baryshevsky</surname><given-names>V. G.</given-names></name></name-alternatives><bio xml:lang="ru"><p>доктор физико-математических наук, профессор, почетный директор, главный научный сотрудник </p><p>ул. Бобруйская, 11, Минск, 220030</p></bio><bio xml:lang="en"><p>D. Sc. (Physics and Mathematics), Professor, Honorary Director, Principal Research Scientist</p><p>11, Bobruiskaya Str., Minsk, 220030</p></bio><email xlink:type="simple">bar@inp.bsu.by</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Тихомиров</surname><given-names>В. В.</given-names></name><name name-style="western" xml:lang="en"><surname>Tikhomirov</surname><given-names>V. V.</given-names></name></name-alternatives><bio xml:lang="ru"><p>доктор физико- математических наук, профессор, заведующий лабораторией</p><p>лаборатория ядерной оптики и космомикрофизики </p><p>ул. Бобруйская, 11, Минск, 220030</p></bio><bio xml:lang="en"><p>D. Sc. (Physics and Mathematics), Professor, Head of the Laboratory of Nuclear Optics and Astroparticle Physics</p><p>11, Bobruiskaya Str., Minsk, 220030</p></bio><email xlink:type="simple">tikh@inp.bsu.by</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Институт ядерных проблем Белорусского государственного университета</institution></aff><aff xml:lang="en"><institution>Institute for Nuclear Problems of the Belarusian State University</institution></aff></aff-alternatives><pub-date pub-type="collection"><year>2017</year></pub-date><pub-date pub-type="epub"><day>23</day><month>01</month><year>2018</year></pub-date><volume>0</volume><issue>4</issue><fpage>20</fpage><lpage>32</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Барышевский В.Г., Тихомиров В.В., 2018</copyright-statement><copyright-year>2018</copyright-year><copyright-holder xml:lang="ru">Барышевский В.Г., Тихомиров В.В.</copyright-holder><copyright-holder xml:lang="en">Baryshevsky V.G., Tikhomirov V.V.</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://vestifm.belnauka.by/jour/article/view/276">https://vestifm.belnauka.by/jour/article/view/276</self-uri><abstract><p>При движении частиц высоких энергий вдоль осей или плоскостей кристалла они испытывают действие протяженного эффективного поля, напряженность которого на порядки превосходит величины, создаваемые любыми стационарными магнитами. Столь сильные поля открывают широкие возможности наблюдения новых явлений, измерения характеристик частиц, управления их пучками, а также генерации и поляризации последних. Многие из этих возможностей были предсказаны белорусскими учеными и наблюдались в ЦЕРН, ФНАЛ, ИФВЭ и других ускорительных центрах. Предложенные эффекты увеличения эффективности захвата частиц в режим каналирования при помощи выреза в кристалле и усиления их отклонения вследствие отражения от различных плоскостей одного кристалла позволяют усилить защиту сверхпроводящих магнитов Большого адронного коллайдера и проектируемого адронного коллайдера Будущего. Значительное усиление процесса излучения и рождения пар в кристаллах может оказывать влияние на функционирование калориметра Компактного мюонного соленоида (CSM) гамма-телескопа «Ферми», а также быть использовано при разработке более эффективных калориметров и гамма- телескопов в будущем. Эффект вращения спина каналированных частиц в изогнутых кристаллах делает возможным измерения магнитных и электрических дипольных моментов короткоживущих очарованных и бьюти-гиперонов, а также наблюдать изменение магнитного момента электрона. </p></abstract><trans-abstract xml:lang="en"><p>When high energy particles move along the crystal axis or plane, they experience the action of an extended effective field, the strength of which by orders of magnitude exceeds that of any stationary magnet. These fields give rise to wide possibilities of new phenomena observation, particle properties measurement, high energy beam control, generation and polarization. Many of their possibilities have been predicted by Belarusian scientists and observed at CERN, FNAL, IHPEP, etc. The revealed effects of channeling efficiency increase by crystal cutting and multiple volume reflection from different atomic planes of the same bent crystal make it possible to improve the radiation protection of superconducting magnets of both the high luminocity Large hardron collider phase and the Future circular collider. A drastic enhancement of both radiation and pair production processes in crystals can influence the functioning of both the existing Compact muon solenoid electromagnetic calorimeter at CERN and Fermi gamma-telescope as well as can be applied to devise more effective calorimeters and gamma-telescopes in future. A remarkable effect of channeling particle spin rotation in bent crystals enables one to measure both magnetic and electron dipole moments of short-lived charm and beauty hyperons as well as to observe electron magnetic moment modification. </p></trans-abstract><kwd-group xml:lang="ru"><kwd>кристалл</kwd><kwd>высокие энергии</kwd><kwd>электрон</kwd><kwd>позитрон</kwd><kwd>гамма-квант</kwd><kwd>сильное поле</kwd><kwd>квантовая электродинамика</kwd><kwd>коллимация</kwd><kwd>излучение</kwd><kwd>рождение пар</kwd><kwd>магнитный момент</kwd></kwd-group><kwd-group xml:lang="en"><kwd>crystal</kwd><kwd>high energies</kwd><kwd>electron</kwd><kwd>positron</kwd><kwd>gamma-quantum</kwd><kwd>strong field</kwd><kwd>quantum electrodynamics</kwd><kwd>collimation</kwd><kwd>radiation</kwd><kwd>pair production</kwd><kwd>magnetic moment</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Baryshevsky V. 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Doi: 10.1016/j.nimb.2017.02.081</mixed-citation></citation-alternatives></ref></ref-list><fn-group><fn fn-type="conflict"><p>The authors declare that there are no conflicts of interest present.</p></fn></fn-group></back></article>
