A Comprehensive Study of Rotating Black Hole Formation as Lattice Fabric Defects in Layered-Spinor Bose-Einstein Cosmology with SU(3) and GR Enhancements

We investigate the formation of a ∼ 3 M⊙ rotating (Kerr) black hole within a speculative layered-spinor Bose-Einstein cosmology (BEC) framework, where black holes emerge as lattice defects in a six-layered spinor fabric. Energy amplification is modeled via 3D lattice simulation incorporating SU(3) vacuum bursts and General Relativity (GR) frame-dragging.We derive the strain–dragging coupling tensor directly from GR stressenergy and a unified coupling law. The resulting amplification reproduces collapse energies to within a factor of ∼ 3 of expectations, while predicting oscillatory signatures testable in gravitational waves. We also propose physically motivated damping mechanisms that yield a realistic ringdown timescale, ensuring the model’s predictions are consistent with observation.