Density-Dependent Gravity and the Internal Structure of Black Holes

This paper discusses recent astronomical observations related to the disruption of stars near black holes and long-lasting energy outbursts. While classical gravitational models successfully describe the observed kinematics, they do not provide a unified physical mechanism explaining the stability of matter and sustained energy release under extreme conditions. Within the Ivashura theory, space is treated as a physical medium filled with dark energy, and gravitation is interpreted as the motion of matter within flows of this energy. The proposed approach explains stellar disruption events and prolonged emission near black holes through a single energetic mechanism associated with a deficit in dark energy density and the vortex structure of its flows. This work develops and extends a phenomenological model previously introduced by the author and can be regarded as a continuation of a series of publications devoted to the Ivashura theory. This paper is directly related to the previous work by the author and represents a continuation of the Ivashura theory framework. See the first paper: FUNDAMENTAL LAW OF GRAVITATION https://zenodo.org/records/18199417 F(r) = K(rho) * (P1 * P2) / r^2