Manuscript Hawk01-B@1 · Hawk01-B.tex · section · cfa976f1
An independently checkable small example
An independently checkable small example · lines 1974–2071
Hawk01-B@1#eq:exampleparameters, Hawk01-B@1#tab:exactexample
Choose
The units here are model energy units, not astrophysical mass or temperature assignments. Then
The endpoint radiation has eight completed-state rails of energy three and eight pending-state rails of energy four. The residual source becomes one vacuum state.
{Exact model outputs. Entropies and mutual informations are in bits. uses a pure code input; uses the maximally entangled reference input. At , is empty.}
| Step | |||||||
|---|---|---|---|---|---|---|---|
| Endpoint |
The Bell-input optimal fidelities are, in order,
The conditional reference-information increments are zero for the key, one bit for attempt two, one-half bit for attempt three, and one-half bit for the endpoint.
The exact mean residual energies are
with the corresponding emitted energy giving total five in every branch, not merely on average.
Destructive number-record recovery gives
These values differ from the coherent-access column in Table tab:exactexample.
thermal comparison. To match the vacuum/one-particle restrictions of the two attempt marginals, solve . This gives
The omitted product-thermal probabilities are
Thus even this simple calibration exposes a large thermal discrepancy at the first attempt. These values are formal comparison parameters, not claims that a Schwarzschild greybody calculation produces them. For the four-rail key block, (eq:keythermalobstruction) gives minimal product-thermal distance
Displayed formulas in this passage
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