We present a novel theoretical framework for predicting the distribution of technological civilizations that is fully consistent with ΛCDM cosmology and existing observational constraints.Unlike previous phenomenological approaches, our model derives civilization density from threefundamental physical factors: (i) the available evolutionary time window, (ii) dynamical stabilityagainst mergers and AGN feedback, and (iii) chemical habitability including planet survival. TheInformational Universe (IU) enters not as an ad hoc amplifier, but as an environmental modulator of structure growth, active only in a specific redshift window (z ∼ 0.8 ± 0.3) and mass range(1011−12M⊙). This formulation naturally suppresses clusters and low-mass halos, yielding a peak in civilization density at Mpeak ≈ 1011.3−11.8M⊙ and z⋆ ≈ 0.8 ± 0.3. The IU enhancement is localized to filamentary, quiescent environments, with nIU/nΛCDM = 1.1 − 1.3 — a falsifiable prediction for next-generation SETI surveys. The framework is designed for numerical implementation via MonteCarlo merger trees and is directly testable with upcoming wide-field technosignature searches.
Mikheil Rusishvili (Tue,) studied this question.