Critical Rotational Frequency for Superfluid Fermionic Gases across a Feshbach Resonance

Details Critical Rotational Frequency for Superfluid Fermionic Gases across a Feshbach Resonance Critical Rotational Frequency for Superfluid Fermionic Gases across a Feshbach Resonance

2006-08-09

arxiv.org/abs/cond-mat/0608233v2

Physical Review Letters, 97, 180414 (2006)

Physics

Condensed Matter

Superconductivity

4 pages, 2 figures, published version

Scientific paper

10.1103/PhysRevLett.97.180414

We present a method to determine the critical rotational frequencies for superfluidity of both uniform and trapped Fermi gases across wide Feshbach resonance. It is found that as one approaches the resonance from the BCS side, beyond a critical scattering length, pairing is so robust that superfluidity cannot be destroyed by rotation. Moreover, the critical frequency has a sequence of jumps revealing the appearance of Landau levels, which are particularly prominent for systems up to a few thousand particles. For rotational frequency below an "ultimate" critical frequency, defined to be the lowest frequency at which the center of the cloud goes normal, a trapped gas has a superfluid core surrounded by a normal gas, as seen in recent experiments.

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