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Dark matter in the Milky Way as the F-type of vacuum polarization.
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Academic Editor: Mauro D'Onofrio
Published:
15 February 2023
by MDPI
in 2nd Electronic Conference on Universe
session Galaxies and Clusters
Abstract:
Dark matter in the Milky Way is explained by the F-type of vacuum
polarization [1], which could be considered as representing dark
radiation. A nonsingular solution for dark radiation exists in the
presence of eicheon (i.e., black hole in old terminology) in the center
of the galaxy [1]. The model is spherically symmetric, but
a surface density of a baryonic galaxy disk is taken into account
approximately by smearing the disk over a sphere.
[1] S.L. Cherkas, V. L. Kalashnikov, Universe -2022. -Vol.8. -P.456.
Keywords: rotational curve; dark matter; vacuum polarization; nonsingular solution for dark radiation
