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Interaction-Driven Instabilities in the Random-Field XXZ Chain
Physical Review Letters ( IF 8.1 ) Pub Date : 2024-09-12 , DOI: 10.1103/physrevlett.133.116502 Jeanne Colbois 1, 2 , Fabien Alet 1, 2 , Nicolas Laflorencie 1, 2
Physical Review Letters ( IF 8.1 ) Pub Date : 2024-09-12 , DOI: 10.1103/physrevlett.133.116502 Jeanne Colbois 1, 2 , Fabien Alet 1, 2 , Nicolas Laflorencie 1, 2
Affiliation
Despite enormous efforts devoted to the study of the many-body localization (MBL) phenomenon, the nature of the high-energy behavior of the Heisenberg spin chain in a strong random magnetic field is lacking consensus. Here, we take a step back by exploring the weak interaction limit starting from the Anderson localized (AL) insulator. Through shift-invert diagonalization, we find that, below a certain disorder threshold , weak interactions necessarily lead to an ergodic instability, whereas at strong disorder the AL insulator directly turns into MBL, in agreement with a simple interpretation of the avalanche theory for restoration of ergodicity. We further map the phase diagram for the generic model in the disorder –interaction plane. Taking advantage of the total magnetization conservation, our results unveil the remarkable behavior of the spin-spin correlation functions: in the regime indicated as MBL by standard observables, their exponential decay undergoes an inversion of orientation . We find that the longitudinal length is a key quantity for capturing ergodic instabilities, as it increases with system size near the thermal phase, in sharp contrast to its transverse counterpart.
中文翻译:
随机场 XXZ 链中交互驱动的不稳定性
尽管付出了巨大的努力 在多体局域化(MBL)现象的研究中,海森堡自旋链在强随机磁场中的高能行为的本质缺乏共识。在这里,我们退后一步,从安德森局域 (AL) 绝缘体开始探索弱相互作用极限。通过移位反转对角化,我们发现,低于某个无序阈值 ,弱相互作用必然导致遍历不稳定性,而在强无序下,AL 绝缘体直接变成 MBL,这与恢复遍历性的雪崩理论的简单解释一致。我们进一步绘制通用相图 h-相互作用障碍模型 飞机。利用总磁化守恒,我们的结果揭示了自旋相关函数的显着行为:在标准可观测量表示为 MBL 的区域中,它们的指数衰减经历了方向反转 。我们发现纵向长度 是捕获遍历不稳定性的关键量,因为它随着热相附近的系统尺寸而增加,与其横向对应物形成鲜明对比。
更新日期:2024-09-12
中文翻译:
随机场 XXZ 链中交互驱动的不稳定性
尽管付出了巨大的努力 在多体局域化(MBL)现象的研究中,海森堡自旋链在强随机磁场中的高能行为的本质缺乏共识。在这里,我们退后一步,从安德森局域 (AL) 绝缘体开始探索弱相互作用极限。通过移位反转对角化,我们发现,低于某个无序阈值 ,弱相互作用必然导致遍历不稳定性,而在强无序下,AL 绝缘体直接变成 MBL,这与恢复遍历性的雪崩理论的简单解释一致。我们进一步绘制通用相图 h-相互作用障碍模型 飞机。利用总磁化守恒,我们的结果揭示了自旋相关函数的显着行为:在标准可观测量表示为 MBL 的区域中,它们的指数衰减经历了方向反转 。我们发现纵向长度 是捕获遍历不稳定性的关键量,因为它随着热相附近的系统尺寸而增加,与其横向对应物形成鲜明对比。