A Physical Model of Black Hole Evolution: Formation to Freeze-Out

We develop a physical model of black hole evolution governed by suppression dynamics. During collapse, suppression increases monotonically toward the center, inducing a center-initiated freezeout whose boundary propagates outward at light speed. Propagation terminates when suppression gradients self-consistently support the configuration, thereby fixing the black hole’s final size. Angular momentum is locked during freeze-out, implying a spin that remains invariant under subsequent accretion. The framework yields a causal account of black hole formation and evolution without relying on horizon-defined or purely symmetry-based constructions.