Kourehpaz Mahdi, Donsa Stefan, Lackner Fabian, Burgdörfer Joachim, Březinová Iva
Institute for Theoretical Physics, Vienna University of Technology, Wiedner Hauptstraße 8-10/136, 1040 Vienna, Austria.
Entropy (Basel). 2022 Nov 29;24(12):1740. doi: 10.3390/e24121740.
One key issue of the foundation of statistical mechanics is the emergence of equilibrium ensembles in isolated and closed quantum systems. Recently, it was predicted that in the thermodynamic (N→∞) limit of large quantum many-body systems, canonical density matrices emerge for small subsystems from almost all pure states. This notion of canonical typicality is assumed to originate from the entanglement between subsystem and environment and the resulting intrinsic quantum complexity of the many-body state. For individual eigenstates, it has been shown that local observables show thermal properties provided the eigenstate thermalization hypothesis holds, which requires the system to be quantum-chaotic. In the present paper, we study the emergence of thermal states in the regime of a quantum analog of a mixed phase space. Specifically, we study the emergence of the canonical density matrix of an impurity upon reduction from isolated energy eigenstates of a large but finite quantum system the impurity is embedded in. Our system can be tuned by means of a single parameter from quantum integrability to quantum chaos and corresponds in between to a system with mixed quantum phase space. We show that the probability for finding a canonical density matrix when reducing the ensemble of energy eigenstates of the finite many-body system can be quantitatively controlled and tuned by the degree of quantum chaos present. For the transition from quantum integrability to quantum chaos, we find a continuous and universal (i.e., size-independent) relation between the fraction of canonical eigenstates and the degree of chaoticity as measured by the Brody parameter or the Shannon entropy.
统计力学基础的一个关键问题是孤立和封闭量子系统中平衡系综的出现。最近,有人预测,在大型量子多体系统的热力学((N→∞))极限下,几乎所有纯态的小子系统都会出现正则密度矩阵。这种正则典型性的概念被认为源于子系统与环境之间的纠缠以及由此产生的多体状态的内在量子复杂性。对于单个本征态,已经证明,只要本征态热化假设成立,局部可观测量就会表现出热性质,这要求系统是量子混沌的。在本文中,我们研究了混合相空间量子模拟区域中热态的出现。具体来说,我们研究了嵌入杂质的大型但有限量子系统的孤立能量本征态约化时杂质正则密度矩阵的出现。我们的系统可以通过一个参数从量子可积性调节到量子混沌,中间对应于具有混合量子相空间的系统。我们表明,在约化有限多体系统的能量本征态系综时找到正则密度矩阵的概率可以通过存在的量子混沌程度进行定量控制和调节。对于从量子可积性到量子混沌的转变,我们发现正则本征态的比例与由布罗迪参数或香农熵测量的混沌程度之间存在连续且通用(即与尺寸无关)的关系。