Synthetic gravitational horizons in low-dimensional quantum matter
arXiv:2104.03875 · doi:10.1103/PhysRevResearch.3.L022022
Abstract
We propose a class of lattice models realizable in a wide range of setups whose low-energy dynamics exactly reduces to Dirac fields subjected to (1+1)-dimensional gravitational backgrounds, including (anti-)de Sitter spacetime. Wave-packets propagating on the lattice exhibit an eternal slowdown for power-law position-dependent hopping integrals when , signalling the formation of black hole event horizons. For instead the wave-packets behave radically different and bounce off the horizon. We show that the eternal slowdown relates to a zero-energy spectral singularity of the lattice model and that the semiclassical wave packets trajectories coincide with the geodesics on (1+1)D dilaton gravity, paving the way for new and experimentally feasible routes to mimic black hole horizons and realize (1+1)D spacetimes as they appear in certain gravity theories.
arXiv comment6 pages, 5 figures
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- Thermalization by a synthetic horizon
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