Krylov Complexity of Open Quantum Systems: From Hard Spheres to Black Holes
arXiv:2308.10945 · doi:10.1007/JHEP11(2023)222
Abstract
We examine the complexity of quasi-static chaotic open quantum systems. As a prototypical example, we analytically compute the Krylov complexity of a slowly leaking hard-sphere gas using Berry's conjecture. We then connect it to the holographic complexity of a -dimensional evaporating black hole using the Complexity=Volume proposal. We model the black hole spacetime by stitching together a sequence of static Schwarzschild patches across incoming negative energy null shock waves. Under certain identification of parameters, we find the late time complexity growth rate during each quasi-static equilibrium to be the same in both systems.
25 pages, 7 figures; v2: refs added, minor changes. Matches the published version
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- Spread and Spectral Complexity in Quantum Spin Chains: from Integrability to Chaos
- Krylov complexity as an order parameter for quantum chaotic-integrable transitions
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- Krylov Complexity of Fermionic and Bosonic Gaussian States
- Generalized CV Conjecture and Krylov Complexity in Two-Mode Hermitian Systems via Information Geometry
- Krylov complexity and Wightman power spectrum with positive chemical potential in Schrödinger field theory