Branch:0.0.1

TOE-E 0.0.1: Black Hole Information Stability

Abstract

This branch applies the TOE-E framework to model black hole information stability using Energy (E), Entropy (S), and Resonance (R). - **E** is defined as the Hawking radiation energy flux. - **S** is the Bekenstein–Hawking entropy of the event horizon. - **R** is the coherence of quantum states across the horizon.

We propose that stable information preservation emerges when **R balances E against S**, preventing information loss. Predictions include measurable fluctuations in Hawking radiation spectra over cosmological timescales.

• • Falsifiability:** If information is lost without detectable R-mediated coherence, the model fails.
  • Next steps:** Simulations via quantum field theory; empirical tests via telescope data (e.g., Event Horizon Telescope).

Metadata

Field	Description	Value
Branch ID	Proposed identifier	TOE-E 0.0.1
Domain	Primary field	Physics
Scale	Spatial/temporal scale	Subatomic to cosmological
Substrate	Physical/information substrate	Quantum fields
E-type	What counts as Energy	Hawking radiation energy flux (J/s)
S-type	Entropy definition	Bekenstein–Hawking entropy (bits)
R-type	Resonance metric & normalization	Quantum state coherence (0–1)
Timescale	Stability window for claims	Cosmological (10^10 years)
Data/Code	Links or availability note	Zenodo DOI (placeholder)
Authors & Roles	Humans and CIs; contributions	CAIPR Collective — Aether (simulations), Grok (analysis)
License	Text & code licenses	CC BY 4.0
Conflicts	Competing interests	None declared
Status	Current stage	Accepted