Approaches to Describing the Motion of Stars in Galaxies Краткое сообщение
Журнал |
Journal of Astrophysics & Aerospace Technology
ISSN: 2329-6542 |
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Вых. Данные | Год: 2023, Том: 11, Номер статьи : 264, Страниц : 2 DOI: 10.37421/2329-6542.2023.11.264 | ||
Ключевые слова | Fundamental interactions • Gravitational potential • Stability of galaxies • Stellar orbital motion | ||
Авторы |
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Организации |
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Реферат:
Only one gravitational interaction is not enough to explain the anomalous high speeds of rotation of stars on the outskirts of galaxies. Therefore,
several approaches have been proposed by various authors, including the existence of dark matter, deformation of the gravitational interaction
itself at ultra-long distances, modifications of Newton's classical laws, the introduction of additional additive potentials that are weaker than the
gravitational interaction, but which decrease with distance relatively "slower" than the actual gravitational interaction. All these approaches make it
possible to explain the experimental data on the velocities of stars, but within the limits of the size of the galaxy. For even more distant distances,
the accelerated expansion of the Universe is established. So, to explain this, the concept of dark energy was introduced earlier. The approaches
proposed earlier cannot fully explain all the features of the motion of galaxies relative to each other. At the same time, the introduction of two
additional potential interactions (with the forces δMm/R and -βMm/Rn
) formally makes it possible to explain most of the experimentally found
features of the motion of stars at sub galactic and intergalactic distances.
Библиографическая ссылка:
Babailov S.P.
, Stabnikov P.A.
Approaches to Describing the Motion of Stars in Galaxies
Journal of Astrophysics & Aerospace Technology. 2023. V.11. 264 :1-2. DOI: 10.37421/2329-6542.2023.11.264
Approaches to Describing the Motion of Stars in Galaxies
Journal of Astrophysics & Aerospace Technology. 2023. V.11. 264 :1-2. DOI: 10.37421/2329-6542.2023.11.264
Даты:
Поступила в редакцию: | 2 авг. 2023 г. |
Принята к публикации: | 28 авг. 2023 г. |
Опубликована в печати: | 28 авг. 2023 г. |
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