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Probing quantum properties of black holes with a Floquet-driven optical lattice simulator
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Probing quantum properties of black holes with a Floquet-driven optical lattice simulator
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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.
Forward citations
Cited by 2 Pith papers
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On the dilaton gravity of analogue black holes
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.
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On the dilaton gravity of analogue black holes
Typical 2D laboratory analogue black holes do not match known dilaton gravity models; reversing the map yields experimental conditions needed to realize those models.
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