Λψ: Retentive Invariants Beyond Dynamical Cosmology
Year: 2026
Type: article
Abstract: This work introduces a post-dynamical interpretative framework for late-time cosmology based on the concept of retention—the capacity of large-scale cosmic structures to preserve form and correlation beyond the phase of active dynamical growth. Motivated by persistent observational tensions, most notably the reduced clustering amplitude quantified by the parameter S_8, the paper proposes a minimal phenomenological invariant, \Lambda_\psi, describing structural persistence rather than dynamical acceleration. The framework does not modify gravity, introduce new particle species, or alter the standard dynamical equations of \LambdaCDM. Instead, it operates as a complementary interpretive layer applicable once large-scale structure formation has effectively saturated. The retentive invariant is formulated to characterize a late-time regime in which cosmic filaments, voids, and correlation patterns exhibit long-term stability despite continued expansion. This regime is identified through model-independent observational criteria, including scale-stable correlations and plateau behavior in clustering amplitudes. A methodological protocol based on the principle of non-violation is introduced to ensure minimal theoretical intrusion in data interpretation. The work emphasizes falsifiability, clearly defined domains of applicability, and explicit interpretive limits. The proposed framework offers a coherent, non-invasive explanation for late-time cosmological anomalies and reframes large-scale structure as a memory-bearing architecture rather than an endlessly evolving dynamical system.
Author: Yulia, Logacheva
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W7123249891
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