V88: First Principles of an Updating Universe — Weak Scaling (β≪1) and Observation Windows

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Authors: Satoshi Yoshida, A. ChatGPT, Gさんからの提案 Gemini, C Claude
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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