This supplemental analysis expands upon the topological framework of the Damascus Topology Model by proposing a novel mechanism for the late-time dynamics of Kerr black hole mergers. While classical models assume post-merger gravitational wave energy radiates away to asymptotic infinity, this analysis hypothesizes that ringdown echoes become geometrically trapped within the Kerr ergosphere. Driven by higher-order nonlinear curvature corrections, these extreme-curvature regions exhibit an emergent, non-uniform flow of time that profoundly alters wave behavior and halts outward propagation.1 Consequently, the trapped gravitational energy is instead channeled along the black hole's geometric future toward future timelike infinity. Integrating these localized dynamics with Roger Penrose's Conformal Cyclic Cosmology (CCC), the framework treats future timelike infinity not as a destructive endpoint, but as a conformal crossover boundary smoothly connecting to the Big Bang of a subsequent cosmic aeon.2 The analysis details how these highly blueshifted, trapped echoes survive the conformal squashing process and pass through this boundary during a transitionary Gravitational Wave Epoch.3 Obeying strict cross-aeon mass-energy conservation laws, the echoes transfer their chaotic, spin-weighted phase-space information directly into the primordial plasma of the new universe.4 Observationally, this mechanism predicts that the structural fingerprints of past-aeon Kerr black holes freeze into the Cosmic Microwave Background (CMB). These crossed-over signals are predicted to manifest as distinct, macroscopic CMB anomalies, including non-Gaussian statistical distributions, subtle phase shifts, and circular temperature ripples spanning approximately 4 degrees across the sky.1, 5 By unifying extreme near-horizon spacetime topology with global cyclical cosmology, this analysis provides a testable, multi-messenger bridge between delayed gravitational wave echoes and observable cosmological artifacts.
Joseph Baughman (Fri,) studied this question.