Black Holes: Dynamics of Nature in Extreme Density with NIT5, a Quantum Field Resolution to Singularities

This work presents a novel theoretical framework— based on the original work, [doi.org/10.5281/zenodo.14997856], Nassimi Interaction Theory (NIT5)—that redefines our understanding of black hole physics. Traditional general relativity predicts singularities and an associated loss of information via Hawking radiation. In contrast, NIT5 introduces a dynamic scalar timefield, Θ, which caps the density at a finite maximum within a Planck-scale core and maintains continuous time evolution through Planck-scale oscillations. This approach not only resolves the classical singularity problem but also offers a potential solution to the Hawking information paradox by enabling information retention and gradual leakage through the oscillatory behavior of Θ. The paper provides detailed derivations of key parameters such as the maximum core density, the oscillation frequency of Θ, and observational predictions including finite redshift near the event horizon and subtle shifts in gravitational wave quasinormal modes. By bridging quantum mechanics and gravitational physics, NIT5 offers a unified description across scales—from the quantum realm to macroscopic astrophysical phenomena—and sets the stage for future multi-messenger observational tests.