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

Back to manuscript

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

  • Hawk01-B@1#eq:exampleparameters · line 1977

  • unlabeled · line 1986

  • unlabeled · line 2025

  • unlabeled · line 2034

  • unlabeled · line 2041

  • unlabeled · line 2053

  • unlabeled · line 2057

  • unlabeled · line 2067