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arXiv · 1802.02703

A strongly interacting Sarma superfluid near orbital Feshbach resonances

Peng Zou·Lianyi He·Xia-Ji Liu·Hui Hu
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Abstract

We investigate the nature of superfluid pairing in a strongly interacting Fermi gas near orbital Feshbach resonances with spin-population imbalance in three dimensions, which can be well described by a two-band or two-channel model. We show that a Sarma superfluid with gapless single-particle excitations is favored in the closed channel at large imbalance. It is thermodynamically stable against the formation of an inhomogeneous Fulde\textendash Ferrell\textendash Larkin\textendash Ovchinnikov superfluid and features a well-defined Goldstone-Anderson-Bogoliubov phonon mode and a massive Leggett mode as collective excitations at low momentum. At large momentum, the Leggett mode disappears and the phonon mode becomes damped at zero temperature, due to the coupling to the particle-hole excitations. We discuss possible experimental observation of a strongly interacting Sarma superfluid with ultracold alkaline-earth-metal Fermi gases.

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Peng Zou, Lianyi He, Xia-Ji Liu, Hui Hu. 2018-02-08. A strongly interacting Sarma superfluid near orbital Feshbach resonances. https://doi.org/10.1103/physreva.97.043616

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