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Then (31) reduces to D∆S log 2 = 2 √ 1− 4ϵ2 2− (1− 4ϵ2

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Modifications of the Page Curve from correlations within Hawking radiation

hep-th · 2019-08-26 · conditional · novelty 5.0

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.

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  • Modifications of the Page Curve from correlations within Hawking radiation hep-th · 2019-08-26 · conditional · none · ref 8

    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.