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Электронный каталог: Silenko, A. J. - Effects of Interactions of Axion-Like Dark Matter with Standard Model Particles
Silenko, A. J. - Effects of Interactions of Axion-Like Dark Matter with Standard Model Particles
Статья
Автор: Silenko, A. J.
Физика элементарных частиц и атомного ядра: Effects of Interactions of Axion-Like Dark Matter with Standard Model Particles : Abstract
б.г.
ISBN отсутствует
Автор: Silenko, A. J.
Физика элементарных частиц и атомного ядра: Effects of Interactions of Axion-Like Dark Matter with Standard Model Particles : Abstract
б.г.
ISBN отсутствует
Статья
Silenko, A.J.
Effects of Interactions of Axion-Like Dark Matter with Standard Model Particles : Abstract / A.J.Silenko // Физика элементарных частиц и атомного ядра. – 2024. – Т. 55, № 6 : XXXV Международное (онлайн) совещание по физике высоких энергий «От кварков до галактик: прояснение темных сторон», Протвино, 28 ноября – 1 декабря 2023 г. : Материалы. – P. 1638. – URL: http://www1.jinr.ru/Pepan/v-55-6/12_Silenko_ann.pdf.
Axion-like dark matter interacts with particles like an axion. The axion is a hypothetical particle being a quant of pseudoscalar field. It was originally postulated by Peccei and Quinn in 1977 to resolve the strong CP problem in QCD. If axions exist, they are of interest as a possible component of cold dark matter. The axion–photon coupling distorts the electromagnetic field and leads to the inverse Primakoff effect which can be observed with haloscopes. The CP noninvariance of the axion–gluon coupling results in an appearance of oscillating nucleon electric dipole moments which are proportional to the axion field. Axions manifest themselves in direct interactions with particles (so-called axion wind effect). We rigorously determine the relativistic spin dynamics defined by the pseudoscalar field of dark matter axions
Спец.(статьи,препринты) = С 324.1д - Квантовая хромодинамика$
ОИЯИ = ОИЯИ (JINR)2024
Silenko, A.J.
Effects of Interactions of Axion-Like Dark Matter with Standard Model Particles : Abstract / A.J.Silenko // Физика элементарных частиц и атомного ядра. – 2024. – Т. 55, № 6 : XXXV Международное (онлайн) совещание по физике высоких энергий «От кварков до галактик: прояснение темных сторон», Протвино, 28 ноября – 1 декабря 2023 г. : Материалы. – P. 1638. – URL: http://www1.jinr.ru/Pepan/v-55-6/12_Silenko_ann.pdf.
Axion-like dark matter interacts with particles like an axion. The axion is a hypothetical particle being a quant of pseudoscalar field. It was originally postulated by Peccei and Quinn in 1977 to resolve the strong CP problem in QCD. If axions exist, they are of interest as a possible component of cold dark matter. The axion–photon coupling distorts the electromagnetic field and leads to the inverse Primakoff effect which can be observed with haloscopes. The CP noninvariance of the axion–gluon coupling results in an appearance of oscillating nucleon electric dipole moments which are proportional to the axion field. Axions manifest themselves in direct interactions with particles (so-called axion wind effect). We rigorously determine the relativistic spin dynamics defined by the pseudoscalar field of dark matter axions
Спец.(статьи,препринты) = С 324.1д - Квантовая хромодинамика$
ОИЯИ = ОИЯИ (JINR)2024