论文标题
反馈冷却的Bose-Einstein凝结:近乎远离平衡
Feedback cooled Bose-Einstein condensation: near and far from equilibrium
论文作者
论文摘要
连续测量的相互作用量子系统几乎总是热量的热量,从而导致量子相干的丧失。在这里,我们研究了经过重复的原子密度测量弱测量的Bose-Einstein冷凝物(BEC),并描述了几种用于生成反馈信号的方案,该反馈信号旨在消除测量反应产生的激发。我们使用随机的Gross-Pitaevskii方程来对系统动力学进行建模,并发现使用动量依赖增益和过滤的反馈协议可以有效地冷却1D和2D系统。这些方案的性能是根据稳态能量,熵和冷凝分数来量化的。这些是在2D中证明的第一个反馈冷却协议,与使用相同方法开发的先前的冷却协议相比,我们的最佳协议将平衡能量降低了100倍以上。我们还使用该方案来从非传递高度激发的状态中淬灭酷1D BEC,并发现它们迅速将其凝结到远离平衡状态,其能量顺序比该凝聚力分数的平衡基态能量高。我们用1D系统的几乎分辨率来解释这一点,从而有效冷却的低动量模式与较高动量模式的能量“储层”有效地解耦。我们观察到,淬灭冷却的凝结状态可以具有量化的超电流描述的非零整数绕组数。
Continuously measured interacting quantum systems almost invariably heat, causing loss of quantum coherence. Here, we study Bose-Einstein condensates (BECs) subject to repeated weak measurement of the atomic density and describe several protocols for generating a feedback signal designed to remove excitations created by measurement backaction. We use a stochastic Gross-Pitaevskii equation to model the system dynamics and find that a feedback protocol utilizing momentum dependant gain and filtering can effectively cool both 1D and 2D systems. The performance of these protocols is quantified in terms of the steady state energy, entropy, and condensed fraction. These are the first feedback cooling protocols demonstrated in 2D, and in 1D our optimal protocol reduces the equilibrium energy by more than a factor of 100 as compared with a previous cooling protocol developed using the same methodology. We also use this protocol to quench-cool 1D BECs from non-condensed highly excited states and find that they rapidly condense into a far from equilibrium state with energy orders of magnitude higher than the equilibrium ground state energy for that condensate fraction. We explain this in terms of the near-integrability of our 1D system, whereby efficiently cooled low momentum modes are effectively decoupled from the energetic `reservoir' of the higher momentum modes. We observe that the quench-cooled condensed states can have non-zero integer winding numbers described by quantized supercurrents.