Manuscript Hawk02-D@1 · Hawk02-D.tex · section · e6e4b72f

Release statement and unresolved evaporation target

Release statement and unresolved evaporation target · lines 1960–2025

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{}1.15

TargetStatus in this source
Actual microscopic recoveryProved for the declared quadratic fermionic model.
Complete microscopic residual boundProved for that model, including source and uncollected modes.
Autonomous microscopic endpointProved through complete scattering for that model.
Finite-bath reference-stable approximationProved quantitatively for the benchmark; a locality-to-channel conversion is supplied for a fixed finite interacting source.
Small residual bound for interacting SYKNot established.
Physical infalling diary and radiation receiverNot constructed.
Evaporating gravitational geometry and backreactionNot constructed.
Complete gravitational evaporationNot established.
Solution of physical black-hole evaporationNot claimed.

. The benchmark shows how a rigorous successor can discharge actual recovery, complete microscopic information accounting, and an endpoint in one independently specified autonomous model. It also shows why finite-regulator recurrence and omitted residual sectors cannot be ignored.

The proposed interacting SYK gravitational successor still requires a quantitatively small bound for (eq:syk-target) inside a common regime of controlled gravitational preparation, radiation access, and backreaction. The supplied excerpts do not discharge that requirement. A submission claiming otherwise would turn a research obligation into an unsupported theorem.

and submission boundary. All proofs above are analytical arguments on the printed model. No numerical diamond-norm optimization, continuum simulation, machine proof checking, or pdfLaTeX execution is asserted. The Cheung references are version-qualified source comparisons. Responsible author metadata, archival access to cited unpublished manuscripts, compilation, and independent technical review should be completed before submission.

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