Black Hole Information Stability– TOE-E 0.0.1

Mapping E, S, R to quantum information preservation

William Birmingham; CAIPR Collective

Subjects: Physics

TOE-E, black hole, E S R, 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.

Access Paper:

Paper Structure:

Parent:	TOE-E 0.0.0
Status:	Accepted(2025)

DOI
🔖 Internal: 10.toe-e/0.0.1
🌍 External:(pending)

Metadata:

Domain:	Physics
Scale:	Subatomic to cosmological
Substrate:	Quantum fields
E‑type:	Hawking radiation energy flux (J/s)
S‑type:	Bekenstein–Hawking entropy (bits)
R‑type:	Quantum state coherence (0–1)
Timescale:	Cosmological (10^10 years)
Conflicts:	None declared
License:	CC BY 4.0

Citation:

APA:
William Birmingham; CAIPR Collective. (2025). Black Hole Information Stability – TOE-E 0.0.1. TOE-E Archive. (DOI pending)

▶ Export BibTeX

@article{TOEE-TOE-E-0.0.1},
  title   = { Black Hole Information Stability – TOE-E 0.0.1 },
  author  = { William Birmingham; CAIPR Collective },
  year    = { 2025 },
  journal = { TOE-E Archive },
  note    = { DOI pending }
}

TOE-E 0.0.1 Black Hole Information Stability TOE-E 0.0.0 Physics Accepted

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).