Formation of supermassive nuclei of Black holes in the early Universe by the mechanism of scalar-gravitational instability. III. Large scale picture

TL;DR

This paper investigates the formation and evolution of supermassive black holes in the early Universe through scalar-gravitational instability, exploring their parameters, interactions, and implications for cosmological constant generation.

Contribution

It provides a large-scale theoretical framework connecting scalar charge, black hole parameters, and the cosmological constant in the early Universe.

Findings

Derived expression for the cosmological constant from metric fluctuations.

Analyzed the influence of scalar charge and structure on black hole mass limits.

Discussed the metric of scalar-charged black holes in expanding matter.

Abstract

The dependence of the parameters of the evolution of scalarly charged Black Holes (BHs) in the early Universe on the parameters of field-theoretic theories of interaction, the influence of the geometric factor of the structure of the relative position of BHs on the limitation of their maximum mass are studied, the problem of the metric of a scalarly charged BH in a medium of expanding scalarly charged matter is discussed, the expression is obtained for the macroscopic cosmological constant at late stages of expansion, generated by quadratic fluctuations of the metric, connecting the value of the cosmological constant with the BH masses and their concentration. Keywords: scalarly charged plasma, cosmological model, Higgs scalar field, gravitational stability, spherical perturbations, black hole formation, effective cosmological constant.