Manuscript Em03-C@1 · Em03-C-v1.tex · section · 47dd71ec
One controlled correction and microscopic dynamics
Open physical bridges: not additional release claims › One controlled correction and microscopic dynamics · lines 2710–2761
A correction successor must choose one theory and specify its action, expansion parameter, state, renormalization, observable, regulator removal, and remainder. Altered classical geometry, interacting matter, graviton loops, and quantum horizon dynamics are different models.
The broader information problem motivates joint-state rather than mean-spectrum questions. Fine-grained radiation entropy calculations EntropyReview are not, by themselves, a complete set of radiation amplitudes or the message channel required in Section sec:information. The horizon-smoothness and unitarity tension AMPS likewise requires hypotheses about interior observables and their relation to exterior radiation. No interior algebra is constructed here.
{}1.12
| Question | Boundary of this construction |
|---|---|
| Microscopic recovery | We supply distinguishability tests; a microscopic input-dependent evaporation channel is absent. |
| Smooth horizon and unitarity | Exterior finite-mode tests do not construct interior partners or decide which locality or factorization hypothesis changes. |
| Gravitational path integrals | No path integral, ensemble identification, or factorization theorem is introduced. |
| Four-dimensional physical correspondence | The field baseline is Schwarzschild scalar radiation; the apparatus-to-local-field bridge remains open. |
| Ultraviolet robustness | No universality class of ultraviolet completions is specified or compared. |
| Evaporation endpoint | The fixed-background model has no Planck-regime endpoint dynamics. |
No result here closes O.1, changes XVI-N's hypotheses, discharges the XIV–XV characteristic-product chain, or admits its separate quantum coefficient. The supplied documentary excerpts about those programmes are not apparatus premises.