We develop a microscopic theory of dynamic structure factor to describe the Bogoliubov-Anderson-
Goldstone phonon mode and its damping rate in a strongly interacting Fermi gas at finite temperature. It is based on a density functional approach - the so-called superfluid local density approximation. The accuracy of the theory is quantitatively examined by comparing the theoretical
predictions with the recent experimental measurements for the local dynamic structure factor of a
nearly homogeneous unitary Fermi gas at low transferred momentum [S. Hoinka et al., Nat. Phys.
13, 943 (2017)], without any free parameters. We calculate the dynamic structure factor as functions of temperature and transferred momentum, and determine the temperature evolution of the
phonon damping rate, by considering the dominant decay process of the phonon mode via scatterings off fermionic quasiparticles. These predictions can be confronted with future Bragg scattering experiments on a unitary Fermi gas near the superfluid transition.
Funding
ARC | FT130100815
ARC | DP170104008
ARC | FT140100003
ARC | DP180102018
Many-Body Localisation of Ultracold Fermionic Atoms in a Dirty Flat Land : Australian Research Council (ARC) | DP170104008
Imbalanced superfluidity with cold atoms: a new way to understand unconventional superconductors and stellar superfluids : Australian Research Council (ARC) | FT130100815
Finding the lost particle: Majorana fermions in ultracold atoms : Australian Research Council (ARC) | FT140100003
Revealing universal exotic superfluidity with ultracold fermionic atoms : Australian Research Council (ARC) | DP180102018