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arXiv 2208.09005cond-mat.stat-mechcond-mat.str-elquant-ph

周期驱动非互易多体自旋系统中的预热化

Prethermalization in periodically-driven nonreciprocal many-body spin systems

Adam J. McRoberts, Hongzheng Zhao, Roderich Moessner, Marin Bukov

AI总结:

本研究针对周期驱动非互易多体自旋系统的动力学特性,提出哈密顿扩展方案推导有效运动方程,将预热动力学概念拓展至非互易系统领域。

摘要:

我们分析了相互作用混沌经典自旋系统中一类新的时间周期非互易动力学,其运动方程是守恒的(保持相空间体积)但不具有辛结构。因此,该系统的动力学无法从任何含时哈密顿量推导得出。在高频极限下,我们发现磁化动力学呈现出长寿命的亚稳态平台,其持续时间由驱动频率的四次方控制。然而,由于缺乏有效哈密顿量,系统演化形成的预热态无法在正则系综框架下理解。我们利用辅助自由度提出了该系统的一个哈密顿扩展方案,其中原始自旋构成一个开放但无耗散的子系统。这使我们能够微扰地推导出有效运动方程,这些方程在频率倒数的领头阶明显表现出辛破缺。由此,我们将在周期驱动系统高频极限中观测到的预热动力学概念拓展到了非互易系统。

英文摘要:

We analyze a new class of time-periodic nonreciprocal dynamics in interacting chaotic classical spin systems, whose equations of motion are conservative (phase-space-volume-preserving) yet possess no symplectic structure. As a result, the dynamics of the system cannot be derived from any time-dependent Hamiltonian. In the high-frequency limit, we find that the magnetization dynamics features a long-lived metastable plateau, whose duration is controlled by the fourth power of the drive frequency. However, due to the lack of an effective Hamiltonian, the prethermal state the system evolves into cannot be understood within the framework of the canonical ensemble. We propose a Hamiltonian extension of the system using auxiliary degrees of freedom, in which the original spins constitute an open yet nondissipative subsystem. This allows us to perturbatively derive effective equations of motion that manifestly display symplecticity breaking at leading order in the inverse frequency. We thus extend the notion of prethermal dynamics, observed in the high-frequency limit of periodically-driven systems, to nonreciprocal systems.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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