Formation of Supermassive Nuclei of Black Holes in the Early Universe by the Mechanism of Scalar-Gravitational Instability. II. Evolution of Localized Spherical Perturbations

被引：0

作者：

Ignat'ev, Yu. G. ^{[1
]}

机构：

[1] Kazan Fed Univ, Inst Phys, Kremlyovskaya Str 16A, Kazan 420008, Russia

来源：

GRAVITATION & COSMOLOGY | 2024年 / 30卷 / 01期

关键词：

D O I：

10.1134/S0202289324010067

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 (SMBH) seeds in the early Universe is studied. Using numerical simulation of the process, it is shown that the mass of SMBH seeds 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.

引用

页码：40 / 47

页数：8

共 13 条

[1] Formation of Supermassive Nuclei of Black Holes in the Early Universe by the Mechanism of Scalar-Gravitational Instability. I. Local Picture
Ignat'ev, Yu. G.
GRAVITATION & COSMOLOGY, 2023, 29 (04): : 327 - 344
[2] Formation of Supermassive Nuclei of Black Holes in the Early Universe by the Mechanism of Scalar-Gravitational Instability. III. Large-Scale Picture
Ignat'ev, Yu. G.
GRAVITATION & COSMOLOGY, 2024, 30 (02): : 141 - 148
[3] Formation of Supermassive Nuclei of Black Holes in the Early Universe by the Mechanism of Scalar-Gravitational Instability. II. Evolution of Localized Spherical Perturbations\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{\mathbf{1}}$$\end{document}
Yu. G. Ignat’ev
Gravitation and Cosmology, 2024, 30 (1) : 40 - 47
[4] Two-Field Model of Gravitational-Scalar Instability and Formation of Supermassive Black Holes in the Early Universe
Ignat'ev, Yu. G.
GRAVITATION & COSMOLOGY, 2023, 29 (02): : 163 - 176
[5] Two-Field Model of Gravitational-Scalar Instability and Formation of Supermassive Black Holes in the Early Universe
Yu. G. Ignat’ev
Gravitation and Cosmology, 2023, 29 : 163 - 176
[6] Single-Field Model of Gravitational-Scalar Instability. II. Black Hole Formation
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GRAVITATION & COSMOLOGY, 2022, 28 (04): : 375 - 381
[7] Single-Field Model of Gravitational-Scalar Instability. II. Black Hole Formation
Yu. G. Ignat’ev
Gravitation and Cosmology, 2022, 28 : 375 - 381
[8] The formation of supermassive black holes from Population III.1 seeds. II. Evolution to the local universe
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Monaco, Pierluigi
Tan, Jonathan C.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 525 (01) : 969 - 982
[9] Formation of supermassive black holes in galactic nuclei - II. Retention and growth of seed intermediate-mass black holes
Askar, Abbas
Davies, Melvyn B.
Church, Ross P.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 511 (02) : 2631 - 2647
[10] Formation of Supermassive Nuclei of Black Holes in the Early Universe by the Mechanism of Scalar-Gravitational Instability. I. Local Picture\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${}^{1}$$\end{document}
Yu. G. Ignat’ev
Gravitation and Cosmology, 2023, 29 (4) : 327 - 344

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