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Main Author: Ignat'ev, Yu. G.
Format: Preprint
Published: 2023
Subjects:
Online Access:https://arxiv.org/abs/2311.09926
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author Ignat'ev, Yu. G.
author_facet Ignat'ev, Yu. G.
contents Based on the previously formulated theory of spherical perturbations in the cosmological medium of self-gravitating scalarly charged fermions with the Higgs scalar interaction and the similarity properties of such models, the formation of supermassive Black Hole Seeds (SSBH) in the early Universe is studied. Using numerical simulation of the process, it is shown that the mass of SSBH during the evolution process reaches a limiting value, after which it begins to slowly fall. The possible influence of nonlinearity on this process is discussed.
format Preprint
id arxiv_https___arxiv_org_abs_2311_09926
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Formation of supermassive nuclei of Black holes in the early\\[8pt] Universe by the mechanism of scalar-gravitational instability. II. The evolution of localized spherical perturbations
Ignat'ev, Yu. G.
General Relativity and Quantum Cosmology
Based on the previously formulated theory of spherical perturbations in the cosmological medium of self-gravitating scalarly charged fermions with the Higgs scalar interaction and the similarity properties of such models, the formation of supermassive Black Hole Seeds (SSBH) in the early Universe is studied. Using numerical simulation of the process, it is shown that the mass of SSBH during the evolution process reaches a limiting value, after which it begins to slowly fall. The possible influence of nonlinearity on this process is discussed.
title Formation of supermassive nuclei of Black holes in the early\\[8pt] Universe by the mechanism of scalar-gravitational instability. II. The evolution of localized spherical perturbations
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2311.09926