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在非周期性驱动的经典旋转系统中进行预热化
Sajag Kumar1, Sayan Choudhury2
1National Institute of Science Education and Research, School of Physical Sciences, a CI of Homi Bhabha National Institute, Jatni 752050, India.
Physical review. E
|February 7, 2025
概括
经典的自旋系统在随机多极驱动下表现出长期存在的预热阶段,随着多极顺序的增加,热化时间会增加. 这种现象比量子系统要慢,为实现时间晶体提供了新的途径.
科学领域:
- 凝聚物质物理学 凝聚物质物理学
- 统计力学 统计力学
- 动态系统 动态系统
背景情况:
- 定期驱动的经典多体系统表现出热前动态阶段.
- 将预热化扩展到非周期性驾驶是一个关键的挑战.
研究的目的:
- 在非周期性驱动的经典旋转系统中研究预热化.
- 在随机多极驱动下确定前热状态的存在和特征.
- 探索经典预热化的潜在应用.
主要方法:
- 对经过随机多极驱动的旋转系统的分析.
- 导出基于多极顺序 (n) 和驱动时间尺度 (T) 的热化时间缩放规律.
- 对各种初始状态能量密度的强度的研究.
主要成果:
- 在具有随机多极驱动的经典自旋系统中建立了长期存在的热前状态.
- 证明热化时间缩放为 (1/T) ^{2n+2},随着多极秩序的增加而增加.
- 在近周期极限 (n→∞) 中观察到指数长的热化时间.
- 确认了预热化到初始状态能量密度的稳定性.
- 值得注意的是,经典的预热化在参数上比量子预热化慢.
结论:
- 在非周期性驱动系统中,可以实现经典的预热化.
- 观察到的缩放定律为预热动力学提供了定量理解.
- 与量子系统相比,经典的预热化提供了一个独特的,可能更慢的途径.
- 提出了一项协议,利用经典的预热化来实现时间晶体.
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