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arXiv 1102.4751cond-mat.quant-gas
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共振费米气体中相互作用的预制库珀对

Interacting Preformed Cooper Pairs in Resonant Fermi Gases

K. B. Gubbels, H. T. C. Stoof

摘要:

我们考虑强相互作用费米气体的正常相位,它可以有一个相等或不等数目的原子在其两个可达的自旋状态。由于不同自旋的粒子之间的吸引相互作用具有么正性限制,形成了非凝聚的库珀对。处理预成电子对的出发点是Nozières-Schmitt-Rink(NSR)理论,该理论将电子对近似为非相互作用的。在这里,我们考虑的库珀对在威尔逊重整化群计划之间的相互作用的影响。从电子对的精确玻色子作用量出发,结合NSR形式和Wilson方法计算了库珀对的自能。我们将我们的发现与Harikoshi { \it et al.} [Science { \bf 327},442(2010)]和Nascimbène { \it et al.} [Nature { \bf 463},1057(2010)],并且发现非常好的一致性。我们还预测人口不平衡的情况下,可以在实验中进行测试。

英文摘要:

We consider the normal phase of a strongly interacting Fermi gas, which can have either an equal or an unequal number of atoms in its two accessible spin states. Due to the unitarity-limited attractive interaction between particles with different spin, noncondensed Cooper pairs are formed. The starting point in treating preformed pairs is the Nozières-Schmitt-Rink (NSR) theory, which approximates the pairs as being noninteracting. Here, we consider the effects of the interactions between the Cooper pairs in a Wilsonian renormalization-group scheme. Starting from the exact bosonic action for the pairs, we calculate the Cooper-pair self-energy by combining the NSR formalism with the Wilsonian approach. We compare our findings with the recent experiments by Harikoshi {\it et al.} [Science {\bf 327}, 442 (2010)] and Nascimbène {\it et al.} [Nature {\bf 463}, 1057 (2010)], and find very good agreement. We also make predictions for the population-imbalanced case, that can be tested in experiments.

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