Black Holes as Topological Defects in a Layered Spinor Bose-Einstein Cosmology

We propose a quantum cosmological framework in which black holes are modeled not as singularities in spacetime, but as topological defects in a layered spinor Bose-Einstein condensate (BEC) evolving on a hyperbolic manifold. Using a modified Gross–Pitaevskii equation (GPE), we simulate wavefunction evolution, defect formation, and energy distribution. Our results reproduce key black hole phenomena—mass, entropy, Hawking radiation, and ringdown frequencies—without invoking classical horizons or singularities. We compare our predictions to the latest gravitational wave data from GW250114 and demonstrate observational consistency. This model offers a coherent, quantized alternative to general relativity’s geometric interpretation of black holes.