Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon

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 Galaxy. That is, the dark matter in the Milky Way Galaxy is explained as the F-type of vacu...

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Main Authors: Sergey L. Cherkas, Vladimir L. Kalashnikov
Format: Article
Language:English
Published: MDPI AG 2023-09-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/9/9/424
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author Sergey L. Cherkas
Vladimir L. Kalashnikov
author_facet Sergey L. Cherkas
Vladimir L. Kalashnikov
author_sort Sergey L. Cherkas
collection DOAJ
description 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 Galaxy. That is, the dark matter in the Milky Way Galaxy 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 Galaxy rotational curve. Andromeda Galaxy’s rotational curve is also discussed.
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spelling doaj.art-41790609410f43139e31e291d30e55fe2023-11-19T13:17:48ZengMDPI AGUniverse2218-19972023-09-019942410.3390/universe9090424Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around EicheonSergey L. Cherkas0Vladimir L. Kalashnikov1Institute for Nuclear Problems, Bobruiskaya 11, 220006 Minsk, BelarusDepartment of Physics, Norwegian University of Science and Technology, 7491 Trondheim, NorwayEicheon 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 Galaxy. That is, the dark matter in the Milky Way Galaxy 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 Galaxy rotational curve. Andromeda Galaxy’s rotational curve is also discussed.https://www.mdpi.com/2218-1997/9/9/424eicheondark mattervacuum polarizationrotational curvegalaxy nuclei
spellingShingle Sergey L. Cherkas
Vladimir L. Kalashnikov
Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
Universe
eicheon
dark matter
vacuum polarization
rotational curve
galaxy nuclei
title Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
title_full Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
title_fullStr Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
title_full_unstemmed Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
title_short Rotational Curves of the Milky Way Galaxy and Andromeda Galaxy in Light of Vacuum Polarization around Eicheon
title_sort rotational curves of the milky way galaxy and andromeda galaxy in light of vacuum polarization around eicheon
topic eicheon
dark matter
vacuum polarization
rotational curve
galaxy nuclei
url https://www.mdpi.com/2218-1997/9/9/424
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AT vladimirlkalashnikov rotationalcurvesofthemilkywaygalaxyandandromedagalaxyinlightofvacuumpolarizationaroundeicheon