Spatiotemporal dynamics of classical and quantum density profiles in low-dimensional spin systems

被引:2
|
作者
Heitmann, Tjark [1 ]
Richter, Jonas [2 ]
Jin, Fengping [3 ]
Michielsen, Kristel [3 ]
De Raedt, Hans [4 ]
Steinigeweg, Robin [1 ]
机构
[1] Univ Osnabruck, Dept Phys, D-49076 Osnabruck, Germany
[2] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[3] Forschungszentrum Julich, Inst Adv Simulat, Julich Supercomp Ctr, D-52425 Julich, Germany
[4] Univ Groningen, Zernike Inst Adv Mat, NL-9747 AG Groningen, Netherlands
来源
PHYSICAL REVIEW RESEARCH | 2022年 / 4卷 / 04期
基金
欧洲研究理事会;
关键词
1D HEISENBERG-MODEL; STATISTICAL-MECHANICS; HYDRODYNAMICS; DIFFUSION; BREAKDOWN; THERMALIZATION; TRANSPORT; MAGNETS; CHAOS;
D O I
10.1103/PhysRevResearch.4.043147
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We provide a detailed comparison between the dynamics of high-temperature spatiotemporal correlation functions in quantum and classical spin models. In the quantum case, our large-scale numerics are based on the concept of quantum typicality, which exploits the fact that random pure quantum states can faithfully approximate ensemble averages, allowing the simulation of spin-1/2 systems with up to 40 lattice sites. Due to the exponentially growing Hilbert space, we find that for such system sizes even a single random state is sufficient to yield results with extremely low noise that is negligible for most practical purposes. In contrast, a classical analog of typicality is missing. In particular, we demonstrate that to obtain data with a similar level of noise in the classical case, extensive averaging over classical trajectories is required, no matter how large the system size. Focusing on (quasi-)one-dimensional spin chains and ladders, we find remarkably good agreement between quantum and classical dynamics. This applies not only to cases where both the quantum and classical models are nonintegrable but also to cases where the quantum spin-1/2 model is integrable and the corresponding classical s -> infinity model is not. Our analysis is based on the comparison of space-time profiles of the spin and energy correlation functions, where the agreement is found to hold not only in the bulk but also in the tails of the resulting density distribution. The mean-squared displacement of the density profiles reflects the nature of emerging hydrodynamics and is found to exhibit similar scaling for quantum and classical models.
引用
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页数:13
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