Manuscript Hawk02-C@2 · Hawk02-C.tex · section · bb332d66
Outstanding gravitational obligations
Physical obligations and unchanged release boundaries › Outstanding gravitational obligations · lines 2443–2478
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:
a physical black-hole code and source degrees of freedom;
a derivation of the autonomous coupling and any excitation-conserving approximation from specified dynamics;
geometry, stress-energy, gravitational energy, and backreaction with a validity domain;
the actual near-horizon state and pair structure;
exterior coupling and dressing independently of any hypothesized interior transfer;
physical packet collection and detector dynamics on complete output spaces;
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.