Dark Stars: Supermassive and Ultramassive Dark Macroobjects ()
ABSTRACT
R. Genzel and A. Ghez were awarded the 2020 Nobel Prize in Physics for their discovery that Sgr A* is a supermassive compact object, for which Supermassive Black Hole (SBH) was the only accepted explanation. In 2013, we proposed a principally different explanation of supermassive compact objects: “Macroobjects of the World have cores made up of the discussed DM particles. Other particles, including DM and baryonic matter, form shells surrounding the cores” [1]. According to the developed Hypersphere World-Universe Model (WUM), the World consists of Dark Matter (about 92.8% of the total Matter) and Ordinary matter (about 7.2%). It means that Dark Matter (DM) should play the main role in any Cosmological model. It is the case in WUM, and Ordinary matter is a byproduct of Dark Matter Particles (DMPs) self-annihilation. In present paper, we discuss Dark Stars, Supermassive and Ultramassive Dark Macroobjects in frames of WUM.
Share and Cite:
Netchitailo, V. (2023) Dark Stars: Supermassive and Ultramassive Dark Macroobjects.
Journal of High Energy Physics, Gravitation and Cosmology,
9, 1021-1043. doi:
10.4236/jhepgc.2023.94075.
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