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It costs nothing to teleport information into a black hole

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arxiv 2504.01058 v2 pith:MLM5GD6U submitted 2025-04-01 hep-th gr-qcquant-ph

classification hep-thgr-qcquant-ph
keywords blackholeenergyinformationcostexteriorqubitthere
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abstract

It is often claimed that adding a qubit to a black hole requires energy $\Delta E \geq T_H \log 2$ so that the extra Bekenstein-Hawking entropy can accommodate the qubit. In this essay, we explain how the recently discovered phenomenon of black hole decoherence allows quantum information to be teleported into a black hole, with arbitrarily small energy cost. The generalized second law is not violated and there is no conflict with unitarity because the teleportation creates new entanglement, analogous to Hawking radiation, between the black hole interior and exterior. In accordance with Landauer's principle, a nonzero minimum energy cost only appears when there is a net erasure of information and noise from the exterior or, equivalently, when ``zerobits'' are sent into the black hole.

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Cited by 2 Pith papers

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

  1. How to Minimize the Decoherence Caused by Black Holes

    hep-th 2025-01 conditional novelty 7.0 of 10

    The optimal continuation of horizon-entangling radiation is a reflected, frequency-filtered copy of the radiation that already fell in, given by a sech convolution kernel.

  2. Black Holes, Entanglement and Decoherence

    hep-th 2025-08 unverdicted novelty 2.0 of 10

    Satishchandran reviews three equivalent mechanisms by which black holes and other Killing horizons decohere nearby quantum superpositions, via interior entanglement, soft radiation, and fluctuating multipoles.

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