V88: First Principles of an Updating Universe — Weak Scaling (β≪1) and Observation Windows
Abstract
We propose that the universe's stability amidst constant fluctuation is not a fine-tuned coincidence but a structural necessity. By modeling the cosmos as a dynamically updating system governed by an Ornstein–Uhlenbeck (OU) universal attractor, we derive the extremely weak scale dependence of effective coupling, γ ∝ N^β with β ≪ 1. This specific scaling arises inevitably from two mechanisms: (i) compression of nominal updates N into effective independent updates N_eff, and (ii) saturation boundaries (black holes and top quarks) acting as runaway brakes. Furthermore, the observed primordial fluctuation amplitude, δρ/ρ ≈ 10⁻⁵, is explained as the "quiet residual" surviving a suppression pipeline. Finally, we introduce the concept of observation windows, proposing that standard physical laws are not absolute truths but stable projections that survive the observational filter.
Fields of Study & Subjects
Cosmology and Gravitation Theories
Advanced Mathematical Theories and Applications
Noncommutative and Quantum Gravity Theories
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 10 January 2026