Seeking sounds of superfluids

At low energies, this energy travels via the collective movement of many particles moving in sync -- essentially, as sound waves -quantified using quasiparticles known as phonons.

Below the superfluid transition temperature T_c these sound waves in a unitary Fermi gas can propagate without collisions and are driven by ripples in the phase of the superfluid order parameter (wave-function) -- this mode is known as the Bogoliubov-Anderson (BA) phonon.

Above T_c, the sound waves become more strongly-damped, and collisions play a dominant role.

Strong similarities were identified in the temperature dependence of sound in the unitary Fermi gas and the behaviour of phonons in liquid helium, which was one of the first superfluids identified historically.

This study provides quantitative benchmarks for dynamical theories of strongly-correlated fermions.

The ultracold atomic gases formed and studied in Prof Chris Vale's lab at Swinburne allow very precise tuning of interactions between atoms.

"We cooled and confined a highly dilute gas of Li⁶ atoms, realising a unitary Fermi gas, which exhibits the strongest interactions allowed by quantum mechanics with a contact potential," explains Prof Vale.

In a unitary gas, elastic collisions become resonant and the thermodynamic properties of the gas become universal functions of the temperature and density. Unitary Fermi gases allow precise testing of theories of interacting fermions.

The team then studied excitations in the gas above and below the superfluid phase transition T_c using two-photon Bragg spectroscopy.

"We measured excitation spectra at a momentum of approximately half the Fermi momentum, both above and below the superfluid critical temperature T_c," explains study author Dr Carlos Kuhn.

Two, focused laser pulses (approx 1.2 milliseconds in duration) intersecting within the gas create a periodic perturbation for the lithium atoms.

Immediately after the twin laser pulse, the confining optical trap is swiT_ched off and the momentum of atoms is measured after 4 milliseconds of expansion, and can be mapped as a function of laser frequency.

The finite duration and size of the Bragg beams lead to a Fourier-limited spectral resolution of approximately 1:25 kHz FWHM which is well below the typical Fermi energies, EF 11 kHz, used in the experiments.