What remains missing for gravity

For a gravitational application, one must still supply:

1. a microscopic complete state and dynamics, with justified radiation and residual algebras or finite encodings;

2. a physical derivation or controlled comparison establishing the required random-state typicality in the relevant conserved sectors;

3. a justified emission clock and radiation-capacity history;

4. a coherent radiation-to-memory receiver with a complete-channel allowance, if recovery is claimed;

5. a same-model endpoint comparison and complete-complement allowance.

Hawking's semiclassical emission calculation is an external field-theoretic result Hawking. The supplied fixed-background emission and En07-C records do not provide these microscopic identifications CheungEm03A,CheungEn07C. A physical mass balance, even if separately supplied, does not construct them.

No finite-band regulator, conditional luminosity law, or independently defined characteristic coefficient is transferred into this model. Existing gravitational Page-curve calculations remain external comparisons, not premises or objects constructed here Penington,AlmheiriEtAl.