Kerr-Schwinger Magnetic Core: Continuum Model and Resolution of the Singularity Paradox

Classical relativistic astrophysics addresses the evolutionary finale of massive stars as avertical gravitational collapse in accordance with the Tolman-Oppenheimer-Volkoff (TOV)limit. Traditional formalism assumes that when neutron degeneracy pressure (Pn) is exceeded, baryonic mass transforms into a space-time anomaly (point singularity) of zero volume and infinite density. However, the absence of physical infinities in nature and the contradiction of symmetric isotropic explosion scenarios—which should be triggered by verticalmetric collapses—with stable relativistic compact object observations necessitate a paradigmatic revision of the standard model. In this study, a new “Cosmic Continuum Model” isdeveloped based on the subatomic hadronic intra-core quantum potential energy, the accumulation dynamics of microscopic energy packets with relativistic effective mass density atthe Planck scale (ℓP ), the regulatory role of extreme angular momentum, and the partnership of trapped magnetic flux (Φ). The transition from a degenerate neutron matrix to anon-baryonic electromagnetic fluid phase is linked via empirical and theoretical parameters.Instead of a “nothingness” at the center of black holes, an ultra-dense, rotating quantummagnetic core (Kerr-Schwinger Magnetic Core) that stabilizes within the limits of conservation laws and quantum field theory is mathematically formulated. Laplacian instabilityproblems in non-linear electrodynamics (NLED) models are overcome by integrating extremespin and Schwinger vacuum polarization tensors. Time-dependent numerical perturbationsimulations confirm dynamic stability at the Planck geometric boundary.