Second sound and the density response function in uniform superfluid atomic gases

TL;DR

This paper reviews how second sound manifests in the density response of superfluid atomic gases, highlighting differences between Bose and Fermi systems and proposing density probes as effective tools for experimental detection.

Contribution

It generalizes the understanding of second sound detection via density response functions in superfluid gases, emphasizing the role of the Landau--Placzek ratio and comparing Bose and Fermi systems.

Findings

The Landau--Placzek ratio influences second sound visibility in Fermi gases.

Second sound has significant spectral weight in density response in strongly interacting Fermi gases.

Differences in first and second sound characteristics between Bose and Fermi superfluids are elucidated.

Abstract

Recently there has been renewed interest in second sound in superfluid Bose and Fermi gases. By using two-fluid hydrodynamic theory, we review the density response $\chi_{nn}(\bq,\omega)$ of these systems as a tool to identify second sound in experiments based on density probes. Our work generalizes the well-known studies of the dynamic structure factor $S(\bq,\omega)$ in superfluid $^4$He in the critical region. We show that, in the unitary limit of uniform superfluid Fermi gases, the relative weight of second vs. first sound in the compressibility sum rule is given by the Landau--Placzek ratio $\lp\equiv (\bar{c}_p-\bar{c}_v)/\bar{c}_v$ for all temperatures below $T_c$. In contrast to superfluid $^4$He, $\lp$ is much larger in strongly interacting Fermi gases, being already of order unity for $T \sim 0.8 T_c$, thereby providing promising opportunities to excite second sound with density probes. The relative weights of first and second sound are quite different in $S(\bq,\omega)$ (measured in pulse propagation studies) as compared to $\mathrm{Im}\chi_{nn}(\bq,\omega)$ (measured in two-photon Bragg scattering). We show that first and second sound in $S(\bq,\omega)$ in a strongly interacting Bose-condensed gas are similar to those in a Fermi gas at unitarity. However, in a weakly interacting Bose gas, first and second sound are mainly uncoupled oscillations of the thermal cloud and condensate, respectively, and second sound has most of the spectral weight in $S(\bq,\omega)$. We also discuss the behaviour of the superfluid and normal fluid velocity fields involved in first and second sound.