Article
Version 2
Preserved in Portico This version is not peer-reviewed
Rotational Curves of the Milky Way and Andromeda in light of Vacuum Polarization around Eicheon
Version 1
: Received: 6 July 2023 / Approved: 12 July 2023 / Online: 12 July 2023 (11:04:30 CEST)
Version 2 : Received: 28 July 2023 / Approved: 16 August 2023 / Online: 16 August 2023 (10:18:35 CEST)
Version 2 : Received: 28 July 2023 / Approved: 16 August 2023 / Online: 16 August 2023 (10:18:35 CEST)
A peer-reviewed article of this Preprint also exists.
Cherkas, S.L.; Kalashnikov, V.L. Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon. Universe 2023, 9, 424. Cherkas, S.L.; Kalashnikov, V.L. Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon. Universe 2023, 9, 424.
Abstract
Eicheon properties are discussed. It is shown that the eicheon surface allows setting a boundary condition for the vacuum polarization and obtaining a solution describing the dark matter tail in the Milky Way. That is, the dark matter in the Milky Way is explained as the F-type of vacuum polarization, which could be treated as dark radiation. The model presented is spherically symmetric, but a surface density of a baryonic galaxy disk is taken into account approximately by smearing the disk over a sphere. This allows the reproduction of the large distance shape of the Milky Way rotational curve. Andromeda's rotational curves are also discussed.
Keywords
eicheon; dark matter; vacuum polarization; rotational curve; galaxy nuclei
Subject
Physical Sciences, Astronomy and Astrophysics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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Commenter: Sergey Cherkas
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