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Manuscript XVII-A@1 · XVII-A.tex · section · 711d7ee4

No interior, entropy–area, or evaporation conclusion

The maps not supplied › No interior, entropy–area, or evaporation conclusion · lines 1058–1077

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The model supplies none of the following:

  • an interior-partner operator or a black-hole interior algebra;

  • an entropy–area relation, a geometric area observable, or an entanglement wedge;

  • a Page curve, an island prescription, Hawking evaporation, backreaction, or an evaporation endpoint;

  • microscopic gravitational dynamics or a quantum coefficient of an inherited gravitational response.

A formal complementary output is not an interior partner. A finite Hilbert-space dimension is not an area. A scalar field equation on a chosen background is not Einstein dynamics. These distinctions are compatible with the broader reconstruction frameworks ADH2015,DHW2016; those frameworks are not assumptions that can silently enlarge Theorem thm:main.