Abstract

This paper refines the cosmic fate scenario of the Time Field Model (TFM) by introducing a dissipation-driven stabilization framework, replacing conventional models of heat death or cosmic bounce. We rigorously model the dissipation rate Γ in TFM's wave-lump dynamics, deriving its evolution from Friedmann equations and local field gradients. Our results predict localized re-expansions (“mini-bangs”) even as global energy decays. Simulations using high-performance computing (HPC) tools—including modified Einstein Toolkit and Boltzmann solvers—indicate observable shifts in the CMB power spectrum and gravitational wave echoes detectable by LISA. These findings unify Planck-scale black hole cores and large-scale cosmic structures under a single mechanism, suggesting the Universe approaches an asymptotic, non-singular end-state—neither collapsing nor decaying into thermal death, but stabilizing through persistent, localized anomalies.