Entropyics 7 : Anisotropy in Cosmic Expansion through Directional Entropy Accumulation (v3)

✔️ This work is licensed under CC BY-ND 4.0. See detailed reproduction notice below. The full manuscript is available in the “Files” section above. ✔️ This paper presents Entropyics 7, a reinterpretation of anisotropy in cosmic expansion using an entropy-based framework. Instead of attributing directional differences in acceleration to local gravitational effects or observational biases, the model proposes that anisotropy arises from uneven cumulative entropy storage in black holes across the sky. ✔️ A directional entropy accumulation model was simulated by partitioning the sky into equal-area regions, assigning synthetic black hole densities and Kerr spin parameters, and calculating entropy ΣS(θ, φ). The model predicts acceleration deviations ∆a(θ, φ) proportional to deviations in entropy storage. ✔️ Regression tests against synthetic anisotropic Hubble residuals yield strong internal consistency (R² ≈ 0.932, slope ≈ 0.922), demonstrating that entropy anisotropy can reproduce directional expansion patterns under controlled simulations. ✔️ This framework suggests that regions with higher black hole entropy density accelerate spacetime flattening more strongly, while entropy-poor regions expand more slowly, creating measurable anisotropy. It offers a testable mechanism for observed H0 directional discrepancies using supernovae, BAO dipole terms, and gravitational wave standard sirens. [Public Reproduction Notice] Licensed under CC BY-ND 4.0. Academic reuse (including summarization, reinterpretation, or translation) is strictly prohibited. Media reproduction — including YouTube, blogs, podcasts, articles, and social platforms — is permitted and encouraged, only with clear attribution to “Y. Jang” and “Entropyics”. Any distortion, misrepresentation, or out-of-context reframing of the theory is strictly prohibited.