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Hayden-Preskill protocol and decoding Hawking radiation at finite temperature

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arxiv 2108.09144 v1 pith:CHSUIJAT submitted 2021-08-20 hep-th gr-qcquant-ph

Hayden-Preskill protocol and decoding Hawking radiation at finite temperature

classification hep-th gr-qcquant-ph
keywords decodingtemperaturefiniteradiationblackhawkinghayden-preskillhole
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the Hayden-Preskill thought experiment at finite temperature and obtain the decoupling condition that the information thrown into an old black hole can be extracted by decoding the Hawking radiation. We then consider the decoding Hayden-Preskill protocol at finite temperature assuming the observer outside the black hole who has the access to the full radiation and the unitary dynamics of the black hole. We also consider the cases when the Hawking radiation has noise and decoherence in the storage. The decoding probabilities and the corresponding fidelities are calculated. It is shown that for all the three cases we have considered, the decoding fidelities are less than unity in general. This result indicates that at finite temperature, the decoding strategy and the recovery algorithm is harder to realize than that at infinite temperature.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Microscopic Side Information Controls Ordered Hayden--Preskill Recovery

    quant-ph 2026-07 conditional novelty 7.0

    Without microscopic position labels, Hayden–Preskill recovery of a fixed diary requires Θ(n^{2/3}) output qubits; coarse block labels reduce this to n^{2/3}B^{-1/3} or n/B.