Pair distribution functions of a superfluid spin-1/2 Fermi gas with contact interactions in the linearized time-dependent BCS theory
Abstract
We show that the minimal mean-field theory to use for calculating the pair distribution functions gσσ'(r,r\,') of a spatially homogeneous, unpolarized spin-1/2 superfluid Fermi gas is not the ordinary static BCS theory, but the linearized time-dependent BCS theory implemented via the fluctuation-dissipation theorem. Indeed, the former completely ignores the acoustic excitation branch - the phonons - of the superfluid, while the latter explicitly takes it into account, as well as the quantum fluctuations induced by the broken-pair continuum. Unlike the first, the second theory (i) reflects the effect of these collective excitations on the system's equation of state, including at zero temperature, (ii) allows the function g(r,r\,') to go at sufficiently large distances strictly below its asymptotic value (/2)2 where is the gas density, as expected according to the quantum hydrodynamics of Landau and Khalatnikov at low temperatures, and (iii) predicts in the function g(r,r\,') at short distances subdominant contributions |r-r\,'|2|r-r\,'| in 3D and |r-r\,'|2(-|r-r\,'|) in 2D, alongside the dominant contributions |r-r\,'| in 3D and |r-r\,'|2|r-r\,'| in 2D already present in static BCS theory but with a lower coefficient. This discussion is relevant to the recent theoretical work of Obeso-Jureidini and Romero-Rochin, and to the ongoing experiments on cold atomic gases at ENS and MIT.
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