Direct proof of the algebraic relative-entropy Page-transition probe in type III factors
Prove that, for evaporating black holes described by type III von Neumann factors, the algebraic relative-entropy probe for the Page transition holds. Concretely, let V be the isometric encoding from the semiclassical code Hilbert space to the full quantum gravity Hilbert space, let \~Ψ and \~Φ be any pair of states on the semiclassical code space and Ψ = V\~Ψ, Φ = V\~Φ their images in the full theory. Show that the differences of Araki algebraic relative entropies D_Rad(t) = (\~Ψ|\~Φ; A_sc^{I∪R}) − (Ψ|Φ; A_qg^{Rad}) and D_BH(t) = (\~Ψ|\~Φ; A_sc^{X}) − (Ψ|Φ; A_qg^{BH}) furnish a valid Page-transition probe in type III factors, namely D_Rad(t) > δ and D_BH(t) > ε for t < t_P, D_Rad(t) = δ and D_BH(t) = ε at t = t_P, and D_Rad(t) ≤ δ and D_BH(t) ≤ ε for t > t_P, for suitable thresholds δ, ε (possibly zero), where (·|·; ·) denotes Araki’s algebraic relative entropy.
References
Although the direct proof of eq:probe2 in type III factors is yet to be established, there are hints for the transfer of information in such cases.
eq:probe2:
$\begin{aligned}
(|;A)-(\Psi|\Phi;A)&\begin{cases}
>\delta, & \text{if $t