Manuscript Hawk02-C@2 · Hawk02-C.tex · section · bb332d66

Outstanding gravitational obligations

Physical obligations and unchanged release boundaries › Outstanding gravitational obligations · lines 2443–2478

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The model has a positive-frequency boson continuum but does not supply a local relativistic field equation, spacetime packet localization, or horizon.

A gravitational successor would need:

  1. a physical black-hole code and source degrees of freedom;

  2. a derivation of the autonomous coupling and any excitation-conserving approximation from specified dynamics;

  3. geometry, stress-energy, gravitational energy, and backreaction with a validity domain;

  4. the actual near-horizon state and pair structure;

  5. exterior coupling and dressing independently of any hypothesized interior transfer;

  6. physical packet collection and detector dynamics on complete output spaces;

  7. endpoint dynamics and a complete residual ledger.

Em03-F's distinct switched model records exterior source imprinting before any hypothesized post-horizon transfer CheungEm03F ({thm:fieldchannel}). A successful source–field bridge therefore does not identify the source as an interior black-hole degree of freedom.

Em03-A's fixed-background emission and underdetermination records do not select this form factor or quantum code CheungEm03A ({thm:main, prop:underdetermination}). Exterior finite-mode tests do not construct interior partners or resolve a firewall problem CheungEm03C. Small-corrections arguments retain their own pair and locality hypotheses Mathur, which are not supplied by calling the present reservoir radiation.