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Probing quantum properties of black holes with a Floquet-driven optical lattice simulator

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arxiv 2312.14058 v4 pith:VIGCP2QM submitted 2023-12-21 cond-mat.quant-gas quant-ph

Probing quantum properties of black holes with a Floquet-driven optical lattice simulator

classification cond-mat.quant-gas quant-ph
keywords blackquantumholeholessimulatoratomscurvedfloquet-driven
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In the curved spacetime of a black hole, quantum physics gives rise to distinctive effects such as Hawking radiation and maximally fast scrambling. Here, we present a scheme for an analogue quantum simulation of (1 + 1) and (2 + 1)-dimensional black holes using ultracold atoms in a locally Floquet-driven optical lattice. We show how the effective dynamics of the driven system can generate position-dependent tunnelling amplitudes that encode the curved geometry of the black hole. Moreover, we provide a simple and robust scheme to determine the Hawking temperature of a (1+1)D simulated black hole based solely on on-site atom population measurements. Combined with the highly tunable onsite atom-atom interactions typical for cold atoms, our simulator provides a powerful and feasible platform to probe the scrambling of quantum information in black holes. We illustrate the ergodicity of our (2+1)D black-hole simulator by showing numerically that its level statistics in the hard-core limit approaches the ergodic regime faster than a globally homogeneous Hamiltonian.

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Forward citations

Cited by 2 Pith papers

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

  1. On the dilaton gravity of analogue black holes

    hep-th 2026-05 unverdicted novelty 5.0

    Typical analogue black holes in superconducting circuits do not match known dilaton gravity models, but known models can be used to derive the lab conditions needed to realize them.

  2. On the dilaton gravity of analogue black holes

    hep-th 2026-05 unverdicted novelty 5.0

    Typical 2D laboratory analogue black holes do not match known dilaton gravity models; reversing the map yields experimental conditions needed to realize those models.