论文标题

费米气体中北极分子转变的热力学特征

Thermodynamic signatures of the polaron-molecule transition in a Fermi gas

论文作者

Parish, Meera M., Adlong, Haydn S., Liu, Weizhe E., Levinsen, Jesper

论文摘要

我们考虑了两个组成部分费米气体的高度自旋影响极限,那里的$ \ downrow $杂质的密度很小,与$ \ uparrow $ fermions的海洋相互作用。在零温度下的单息极限中,存在所谓的二极子分子过渡,其中杂质通过在足够强的吸引力上结合$ \ uparrow $ fermion来急剧改变其特征。使用最近开发的变分方法,我们计算了杂质的热力学特性,并且我们表明,由于杂质光谱函数中激发态的热占用,在有限温度下过渡成为平稳的交叉。然而,在动量分辨的光谱函数中,单个突破性跃迁的残余物原理可以通过拉曼光谱法探测。我们进一步表明,棕褐色的接触表现出特征性的非单调依赖性对温度的依赖性,该依赖性提供了零温极偏振子 - 分子转变的特征。对于有限的杂质密度,我们认为纯粹基于费米极化子的行为的描述是无效的,因为杂质之间的相关性不容忽视。特别是,我们表明,由于$ \ uparrow \ uparrow \ downarrow $分子在费米海引起的$ \ uparrow \ downrow $分子之间的吸引力很强,因此旋转状态的系统在低温下进行了相位分离。因此,我们发现杂质光谱和诱导的杂质 - 障碍性相互作用是理解自旋损伤性费米气体的相图的关键。

We consider the highly spin-imbalanced limit of a two-component Fermi gas, where there is a small density of $\downarrow$ impurities attractively interacting with a sea of $\uparrow$ fermions. In the single-impurity limit at zero temperature, there exists the so-called polaron-molecule transition, where the impurity sharply changes its character by binding a $\uparrow$ fermion at sufficiently strong attraction. Using a recently developed variational approach, we calculate the thermodynamic properties of the impurity, and we show that the transition becomes a smooth crossover at finite temperature due to the thermal occupation of excited states in the impurity spectral function. However, remnants of the single-impurity transition are apparent in the momentum-resolved spectral function, which can in principle be probed with Raman spectroscopy. We furthermore show that the Tan contact exhibits a characteristic non-monotonic dependence on temperature that provides a signature of the zero-temperature polaron-molecule transition. For a finite impurity density, we argue that descriptions purely based on the behavior of the Fermi polaron are invalid near the polaron-molecule transition, since correlations between impurities cannot be ignored. In particular, we show that the spin-imbalanced system undergoes phase separation at low temperatures due to the strong attraction between $\uparrow\downarrow$ molecules induced by the Fermi sea. Thus, we find that the impurity spectrum and the induced impurity-impurity interactions are key to understanding the phase diagram of the spin-imbalanced Fermi gas.

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