Adyghe Int. Sci. J. Vol. 24, No. 1. P. 45–48.
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DOI: https://doi.org/10.47928/1726-9946-2024-24-1-45-48
EDN: JTGXYL
PHYSICS
MSC 85A04 | Original Article |
Rotation of a spiral galaxy without dark matter
Rekhviashvili Sergo Shotovich
Doctor of Physical and Mathematical Sciences, expert of the Higher Attestation Commission in physics, deputy. Director for Research of the Institute of Applied Mathematics and Automation of the Kabardino-Balkarian Scientific Center of the Russian Academy of Sciences, Full member of AIAS, ORCID: 0000-0003-1514-857X (Nalchik, Kabardino-Balkarian Republic, Russia), rsergo@mail.ru
Abstract. The star emits electromagnetic waves intensely, so its motion must be different from that of the planet. Centripetal acceleration during star rotation around the galactic center and the resulted radiation reaction friction creates a valid alternative to the dark matter concept.
Keywords: radiation friction, dark matter, spiral galaxy.
Funding. The work was not carried out within the framework of funds.
Competing interests. There are no conflicts of interest regarding authorship and publication.
Contribution and Responsibility.The author participated in the writing of the article and is fully responsible for submitting the final version of the article to the press.
For citation. Rekhviashvili S. Sh. Rotation of a spiral galaxy without dark matter. Adyghe Int. Sci. J. 2024. Vol. 24, No. 1. Pp. 45–48. DOI: https://doi.org/10.47928/1726-9946-2024-24-1-45-48; EDN: JTGXYL.
Submitted 02.12.2023; approved after reviewing 29.02.2024; aeeepted for publication 20.03.2024.
© Rekhviashvili S. Sh., 2024
REFERENCES
1. Griffiths D. J. Introduction to electrodynamics. 3rd ed. Prentice Hall (1999).
2. de Blok W. J. G., Bosma A. High-resolution rotation curves of low surface brightness galaxies. Astronomy and Astrophysics. 385(3), 816–846 (2002).
3. Tully R. B., Fisher J. R. A new method of determining distances to galaxies. Astronomy and Astrophysics. 54(3), 661–673 (1977).
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