On the internal structure of supermassive compact celestial bodies

Abstract

The conceptual part of the physics of baryonic protomatter and the alternative approach to understanding the internal structure of highly compact stationary supermassive celestial bodies were previously suggested in [1–5]. There are a number of advantages to this approach, which differs in principle from the standard black hole accretion models and is in good agreement with the observational data from active galactic nuclei. In order to be more consistent and convinced in the correctness of previously drawn statements, in our research it has been advantageous to verify them by expansion of the basic ideas with the appropriate and consistent theoretical constructions backed up by detailed numerical studies of the models, which are physically more realistic, with the spherical-symmetric distribution of matter in many-phase stratified states. Multiple integrations in the aftermath prove the validity of the previous physical scenario and correctness of drawn statements that the process of inner distortion of the space-time continuum just serves as the eligible mechanism counteracting to collapse.