在远离平衡的旋转波斯气体中观察宇宙动力学
Maximilian Prüfer1, Philipp Kunkel2, Helmut Strobel2
1Kirchhoff-Institut für Physik, Universität Heidelberg, Heidelberg, Germany. universaldynamics@matterwave.de.
Nature
|November 9, 2018
概括
研究人员观察到远离平衡的量子系统中的宇宙动力学. 这一发现在超冷气体中得到证实,揭示了非热固定点,并对宇宙学和量子色力学产生影响.
科学领域:
- 量子物理学
- 多体系统
- 普遍性
背景情况:
- 预测远离平衡的量子系统是理论物理学中的一个重大挑战.
- 普遍性描述了系统如何对微观细节变得不敏感,在时空进化中表现出缩放.
- 之前的研究探讨了宇宙学和量子色力学中的普遍性,但量子多体系统中缺乏实验证据.
研究的目的:
- 在量子多体系统中实验证明宇宙动力学.
- 为了研究远离平衡的时空演变的缩放性质.
- 确定这些动态的新出现的保存量和运输机制.
主要方法:
- 使用准一维旋转波斯-爱因斯坦凝聚剂进行模拟量子模拟.
- 评估空间解析的旋转相关性以观察动态.
- 从长进化时间的旋转激发相关性中提取了缩放特性.
主要成果:
- 在量子系统中观察到宇宙动态的出现.
- 已确定的动力学由一个新兴的保存量和旋转激发传输到低动量.
- 独立于初始条件的非热缩放行为,表明没有微调.
结论:
- 建立了一类非静止系统,表现出时间独立的扩展指数和函数,表明非热固定点.
- 实验方法为研究非热通用性类提供了一个平台.
- 通过超冷气体实验,这些发现为宇宙学和量子色态学的基本动力学提供了见解.
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