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Yan, H., Ma, Z., Ling, C., Cheng, C. and Huang, J.-S. (2022) First Batch of z ≈ 11-20 Candidate Objects Revealed by the James Webb Space Telescope Early Release Observations on SMACS 0723-73. The Astrophysical Journal Letters, 942, Article No. L9.
https://doi.org/10.3847/2041-8213/aca80c

has been cited by the following article:

• TITLE: Dark Stars: Supermassive and Ultramassive Dark Macroobjects

  AUTHORS: Vladimir S. Netchitailo

  KEYWORDS: World-Universe Model, Dark Stars, Superclusters, Multicomponent Dark Matter, Explosive Volcanic Rotational Fission, Angular Momentum, JWST Discoveries

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.9 No.4, September 28, 2023

  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.