The Al-Shobaki Echo Phenomenon: Definitive Numerical Evidence for Signal Survival Beyond the Event Horizon in Extended Zero Theory 4.0

General Relativity (GR) predicts spacetime singularities at the centers of black holes, where the laws of physics break down and signals cease at the event horizon in what is known as the 'eternal silence'. We present here a comprehensive numerical simulation of Extended Zero Theory 4.0 (EZT 4.0), which resolves the singularity by replacing it with the physical π-Ring structure. Our results, obtained from a series of simulations of a rotating (Kerr-π) black hole, reveal an absolute behavioral gap between the theories. While GR simulations consistently show signal termination, EZT 4.0 simulations record numerous surviving pulses with clear amplitude modulation. Our primary simulation demonstrates a survival of 12 pulses with a standard deviation of 0.305 and a massive time difference of 0.234 seconds. Furthermore, we introduce the "Kerr-π Phase Diagram," which maps the dependence of this echo phenomenon on the black hole's spin parameter, showing a monotonic increase in signal survival from 8 to 59 pulses as spin increases from a=0.1 to a=0.9. This numerical signature of the 'Al-Shobaki Echo Phenomenon' represents definitive evidence for information survival and physical interaction within what was thought to be a forbidden region, opening the door to new black hole physics and establishing EZT 4.0 as a leading candidate to describe reality at its limits.