Mitigating Fermion Hole Heating

A preprint of our recent work investigating the interplay between heating of fermionic atoms and the extended geometry of a “dimple” trap is now available on the arXiv. This work is an important part of our efforts to achieve conditions needed to investigate unconventional superfluid phases in ultracold Fermi gases.

Mitigating Heating of Degenerate Fermions in a Ring-Dimple Atomic Trap (arxiv.org)

Persistent currents in rings of ultracold fermionic atoms

We have produced persistent currents of ultracold fermionic atoms trapped in a toroidal geometry with lifetimes greater than 10 seconds in the strongly-interacting limit. These currents remain stable well into the BCS limit at sufficiently low temperature. We drive a circulating BCS superfluid into the normal phase and back by changing the interaction strength and find that the probability for quantized superflow to reappear is remarkably insensitive to the time spent in the normal phase and the minimum interaction strength. After ruling out the Kibble-Zurek mechanism for our experimental conditions, we argue that the reappearance of superflow is due to long-lived normal currents and the Hess-Fairbank effect.

(arXiv preprint)

Persistent Currents in a Molecular BEC of Fermions

We have just shown that we can clearly distinguish between a ring with a persistent current flowing around it and a stationary superfluid (molecular BEC of Li-6). The basic procedure is to relax the radial confinement of the atoms in the ring trap in a prescribed way, then suddenly release the atoms completely and allow the cloud to expand for several milliseconds. If there is (quantized) circulation around the ring then we see a hole in the middle of the expanded cloud, because of the phase singularity that must be present in the superfluid.

For comparison, if there is no circulation in the superfluid, then the expanded cloud looks like this:

Detecting the vortex signature in this expanding fermionic superfluid is a little more challenging to do well than in previous experiments with atomic Bose condensates (of e.g. rubidium or sodium). The cloud expands quite rapidly even for small numbers of atoms, because the momentum of the atoms is comparatively high due to degeneracy pressure. We’ve got a handle on this, though and it’s clearly not going to be an obstacle to the experiments we have planned. The images above mostly look noisy due to photon shot noise, and we expect to be able to do much better than this soon.