Gravitational Tunneling via Inertial Snap-Through and Cosmogenesis: An Evolutionary Model of Eccentric Dark Matter Distributions

Title Gravitational Tunneling via Inertial Snap-Through and Cosmogenesis: An Evolutionary Model of Eccentric Dark Matter Distributions Description Abstract This paper presents a dynamical model of gravitational collapse that extends the analytic continuation of the Schwarzschild metric to address the singularity problem in classical General Relativity. By incorporating spin-torsion coupling (Einstein-Cartan Theory), we propose a "Snap-through Instability" mechanism—analogous to mechanical hairpin buckling. This mechanism posits that collapsing matter possesses sufficient inertial momentum to overcome the potential barrier at $r=0$, acting as activation energy that drives a topological phase transition. Instead of terminating in a singularity, the collapse tunnels into a negative manifold region ($r