Journal of High Energy Physics, Gravitation and Cosmology

Volume 9, Issue 4 (October 2023)

ISSN Print: 2380-4327   ISSN Online: 2380-4335

Google-based Impact Factor: 1.31  Citations  

Dark Stars: Supermassive and Ultramassive Dark Macroobjects

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DOI: 10.4236/jhepgc.2023.94075    68 Downloads   263 Views  

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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.

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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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