Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.
Nature. 2011 Apr 14;472(7342):201-4. doi: 10.1038/nature09989.
Transport of fermions, particles with half-integer spin, is central to many fields of physics. Electron transport runs modern technology, defining states of matter such as superconductors and insulators, and electron spin is being explored as a new carrier of information. Neutrino transport energizes supernova explosions following the collapse of a dying star, and hydrodynamic transport of the quark-gluon plasma governed the expansion of the early Universe. However, our understanding of non-equilibrium dynamics in such strongly interacting fermionic matter is still limited. Ultracold gases of fermionic atoms realize a pristine model for such systems and can be studied in real time with the precision of atomic physics. Even above the superfluid transition, such gases flow as an almost perfect fluid with very low viscosity when interactions are tuned to a scattering resonance. In this hydrodynamic regime, collective density excitations are weakly damped. Here we experimentally investigate spin excitations in a Fermi gas of (6)Li atoms, finding that, in contrast, they are maximally damped. A spin current is induced by spatially separating two spin components and observing their evolution in an external trapping potential. We demonstrate that interactions can be strong enough to reverse spin currents, with components of opposite spin reflecting off each other. Near equilibrium, we obtain the spin drag coefficient, the spin diffusivity and the spin susceptibility as a function of temperature on resonance and show that they obey universal laws at high temperatures. In the degenerate regime, the spin diffusivity approaches a value set by [planck]/m, the quantum limit of diffusion, where [planck]/m is Planck's constant divided by 2π and m the atomic mass. For repulsive interactions, our measurements seem to exclude a metastable ferromagnetic state.
费米子(自旋为半整数的粒子)的输运在许多物理领域中都至关重要。电子输运推动了现代技术的发展,定义了超导和绝缘等物质状态,而电子自旋则被探索为信息的新载体。中微子输运为超新星爆炸提供能量,超新星是一颗垂死恒星坍缩的结果,而夸克-胶子等离子体的流体输运则控制了早期宇宙的膨胀。然而,我们对这种强相互作用费米子物质的非平衡动力学的理解仍然有限。费米原子的超冷气体为这类系统提供了一个原始的模型,可以用原子物理学的精度实时进行研究。即使在超导转变之上,当相互作用被调谐到散射共振时,这种气体也会以几乎完美的流体形式流动,具有非常低的粘性。在这种流体动力学状态下,集体密度激发的阻尼很弱。在这里,我们实验研究了(6)Li 原子费米气体中的自旋激发,发现与之相反,它们的阻尼最大。通过空间分离两个自旋分量并在外部俘获势中观察它们的演化,可以感应出自旋电流。我们证明相互作用可以强到足以反转自旋电流,具有相反自旋的分量会相互反射。在近平衡状态下,我们获得了自旋拖曳系数、自旋扩散率和自旋磁化率作为温度的函数,在共振处并展示了它们在高温下遵循普遍规律。在简并状态下,自旋扩散率接近由[planck]/m 设定的值,即扩散的量子极限,其中[planck]/m 是普朗克常数除以 2π,m 是原子质量。对于排斥相互作用,我们的测量似乎排除了亚稳态铁磁状态的存在。