Strongly interacting Sarma superfluid near orbital Feshbach resonances

15Citations
Citations of this article
8Readers
Mendeley users who have this article in their library.

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-Ferrell-Larkin-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.

Cite

CITATION STYLE

APA

Zou, P., He, L., Liu, X. J., & Hu, H. (2018). Strongly interacting Sarma superfluid near orbital Feshbach resonances. Physical Review A, 97(4). https://doi.org/10.1103/PhysRevA.97.043616

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free