Supermassive Black Holes in Young Galaxy

Petro Olexiyovych Kondratenko*

Received : August 20, 2026 | Published : September 07, 2026

Citation: Kondratenko, P. O., “Supermassive Black Holes in Young Galaxy,” Phys. J. Theor. Exp. Stud. 2(3), 1–5 (2026). DOI: 10.64978/pjtes.2026.0907014

License: This article is licensed under a Creative Commons Attribution 4.0 International License (CC BY 4.0) , which permits use, sharing, adaptation, distribution, and reproduction in any medium or format, provided appropriate credit is given to the original author(s) and the source, a link to the Creative Commons licence is provided, and any changes made are indicated.

Abstract

The article considers the mechanism for creating massive black holes in young galaxies within the framework of the model of the Universe with minimum initial entropy (UMIE). It shows that galaxies form immediately after the Universe begins loading with matter. In this case, matter enters the Universe at a constant speed, increasing the mass of star embryos. The initial distance between the planes of galaxies is of the order of 0.1 m. At the same time, uncertainties in the initial coordinates of star embryos and galaxies, which are described by the Gaussian function, can be 0.02-0.05 m. This can cause several galaxies to merge, producing massive stars and massive central black holes in young galaxies. Unique cases are possible when the merged galaxies merge again, creating several massive holes.

Keywords: The UMIE model, the embryos of stars and galaxies, the merger of galaxy embryos, the creation of massive black holes in young galaxies.