Horizon Area Invariance in Nodal Theory — Q.E.D. S11
10/24/2025
2510243471119

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Publisher: Zenodo
DOI: https://doi.org/10.5281/zenodo.17433154
License: Creative Commons Attribution 4.0 International (CC BY 4.0)
Description:
First published via Zenodo under the DOI above.
This preprint demonstrates that in the Nodal Theory of Everything (TTN), black holes act as structural reorganization zones where coherence density Φ dominates over radiative flux.
The Q.E.D. S11 establishes that the total curvature integral of a gravitational horizon, ∫ Σ_H κ dA, remains invariant under coherent evolution (collapse or Hawking-like evaporation).
This extends the classical area theorem, interpreting apparent area loss as curvature redistribution along the structural axis τ instead of information destruction.
Analytical derivations and numerical validations confirm conservation of the invariant I_H = ∫ κ dA = const within < 2.5 % error.
All rights reserved under CC BY 4.0, preserving full attribution to the author.
Copyright: © 2025 Miguel Jorge Díaz Luna (TTN Project). All rights reserved.

Technical
qed s11
black holes
horizon area
curvature invariance
structural dynamics
hawking radiation
ttn
nodal theory

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Title Horizon Area Invariance in Nodal Theory — Q.E.D. S11
Publisher: Zenodo
DOI: https://doi.org/10.5281/zenodo.17433154
License: Creative Commons Attribution 4.0 International (CC BY 4.0)
Description:
First published via Zenodo under the DOI above.
This preprint demonstrates that in the Nodal Theory of Everything (TTN), black holes act as structural reorganization zones where coherence density Φ dominates over radiative flux.
The Q.E.D. S11 establishes that the total curvature integral of a gravitational horizon, ∫ Σ_H κ dA, remains invariant under coherent evolution (collapse or Hawking-like evaporation).
This extends the classical area theorem, interpreting apparent area loss as curvature redistribution along the structural axis τ instead of information destruction.
Analytical derivations and numerical validations confirm conservation of the invariant I_H = ∫ κ dA = const within < 2.5 % error.
All rights reserved under CC BY 4.0, preserving full attribution to the author.
Copyright: © 2025 Miguel Jorge Díaz Luna (TTN Project). All rights reserved.
Work type Technical
Tags qed s11, black holes, horizon area, curvature invariance, structural dynamics, hawking radiation, ttn, nodal theory

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Identifier 2510243471119
Entry date Oct 24, 2025, 12:42 PM UTC
License All rights reserved

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Author 100.00 %. Holder Miguel Jorge Diaz Luna. Date Oct 24, 2025.


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