论文标题
重力 - 量表不稳定性的单场模型。 ii。黑洞形成
Single-Field Model of Gravitational-Scalar Instability. II. Black Hole Formation
论文作者
论文摘要
基于统计系统的先前制定的数学模型，基于宇宙学模型的标量尺度不稳定性的理论，基于宇宙学模型的重力 - 基于一个组成型的统计统计系统的标量统计系统（\ mio模型）的可能性，使用了早期的大学生在exportiant of the expient of the expient expient of the expient of the Graventition of the机构中的可能性的可能性。扰动。研究了球形质量在\ mio模型中的演变，以及以蒸发量的允许的黑洞的演变。给出了提出的机制在早期宇宙中形成黑洞的可能性的论点，并构建了一个数值模型来证实这一论点。 \ MIO模型的参数范围可确保早期宇宙中黑洞的生长，最高$ 10^4 \ div10^6 m_ \ odot $。
On the basis of the previously formulated mathematical model of a statistical system with scalar interaction of fermions and the theory of gravitational-scalar instability of a cosmological model based on a one-component statistical system of scalarly charged degenerate fermions (\MIO models), the possibility of the formation of black holes in the early Universe using the mechanism of gravitational-scalar instability, which ensures the exponential growth of perturbations. The evolution of spherical masses in the \MIO model, as well as the evolution of black holes with allowance for their evaporation, is studied. The argumentation of the possibility of the formation of black holes in the early Universe with the help of the proposed mechanism is given, and a numerical model is constructed that confirms this argumentation. The range of parameters of the \MIO model, which ensures the growth of black hole masses in the early Universe up to $10^4\div10^6 M_\odot$, is identified.
