For a qubit model of Bell-pair Hawking emission, the per-step change in radiation entanglement entropy is bounded between (1-4*epsilon2^2-sqrt(1-gamma^2))*log2 and sqrt(1-4*epsilon2^2)*log2, yielding an early Page-curve turnover that is incompatible with unitary evaporation.
Time evolution of the hole, will push this matter far along spacelike slices inside the hole such that it is far from where Hawking radiation is being produced
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Modifications of the Page Curve from correlations within Hawking radiation
For a qubit model of Bell-pair Hawking emission, the per-step change in radiation entanglement entropy is bounded between (1-4*epsilon2^2-sqrt(1-gamma^2))*log2 and sqrt(1-4*epsilon2^2)*log2, yielding an early Page-curve turnover that is incompatible with unitary evaporation.