Distortion and Heating an Accretion Disc of a Black Hole

In this work, several properties and phenomena associated with black holes are investigated, including their spinning speed, frequency, angular momentum, and rotational kinetic energy. The study examines how the radius, density, surface temperature, thermal energy, and rotational speed of both the black hole singularity and its accretion disc can rapidly increase or decrease according to conservation laws of angular momentum and energy. It proposes that translational and rotational kinetic energy of particles in the accretion disc is thermalized, and that intense pressure near the singularity can squeeze nuclear fusion material into “superparticles.” Gas and dust are argued to spin up quickly, forming a fast‑orbiting accretion disc that can be distorted and heated by the singularity, superparticles, and nearby celestial objects. The work further suggests that gravitational waves and turbulent superparticles can ripple through the event horizon and disc, tearing matter apart or generating powerful jets, while tidal interactions with celestial objects drive additional disruptions and mass transfer. Finally, it is claimed that the singularity radius is compressed to atomic scales by gravity but is prevented from further collapse and evaporation by thermal energy, superparticle degeneracy pressure, and hydrostatic balance.