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 |