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University of Cambridge > Talks.cam > Theory of Condensed Matter > Emergent Black Hole Dynamics in Critical Floquet Systems
Emergent Black Hole Dynamics in Critical Floquet SystemsAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Katarzyna Macieszczak. While driven interacting quantum matter is generically subject to heating and scrambling, certain classes of systems evade this paradigm. I will discuss such an exceptional class in periodically driven critical (1 + 1)-dimensional systems with a spatially modulated, but disorder-free time evolution operator. Instead of complete scrambling, the excitations of the system remain well-defined. Their propagation is analogous to the evolution along light cones in a curved space-time obtained by two Schwarzschild black holes. The Hawking temperature serves as an order parameter which distinguishes between heating and non-heating phases. Beyond a time scale determined by the inverse Hawking temperature, excitations are absorbed by the black holes resulting in a singular concentration of energy at their center. I will discuss how these results can be obtained analytically within conformal field theory and complementary by means of numerical calculations for an interacting XXZ spin-1/2 chain. The latter demonstrate that our findings are surprisingly robust and survive lattice regularization. This talk is part of the Theory of Condensed Matter series. This talk is included in these lists:
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