Assume that we have an electrically neutral interacting gas (or liquid) of Bose or Fermi particles in a superfluid state. For simplicity, assume that the particles interact via an assigned central potential (the fact that the particles may have integer or half-integer spin is irrelevant to the mutual interaction).
If the system is bosonic, then it should have a repulsive interaction between particles, so that it is "stable" and its Landau critical velocity is bigger than zero (the non-interacting Bose gas is not superfluid because its Landau critical velocity is zero). On the contrary, for a Fermi system, the interaction should be attractive, so we can form Cooper pairs that form the condensate.
Question: provided that the Cooper pairing of the Fermi system has total spin $S=0$ (like in standard BCS), which are the qualitative differences between a Fermi and a Bose superfluid close to absolute zero? Can we expect differences in the nature of the quasiparticles and collective modes? Any good reference to some specialized article or book that makes a clear comparison between the Bose and Fermi cases?
"Close to absolute zero" means that $T \ll T_c$, where $T_c$ is the critical temperature for the superfluid transition. I am asking about that hydrodynamic behaviour because I know that the Tisza-Landau model works for $^4$He, but I am not sure if (and how) it can be derived for a Fermi system.
Comments: let me quickly summarize the info in the comments. At very low energy, the elementary excitations for both cases (Fermi and Bose) are Goldstone modes that should be bosonic collective modes ("phonons"). The high-energy part of the spectrum is not universal (e.g., if the interaction in the Bose system is strong, like in liquid $^4$He, then there may be roton minimum). At the moment the Fermi case is less clear to me (both the low-energy and high-energy parts). In fact: if the phonon-like dispersion relation is valid at low-energy also for the Fermi case, where is the famous "gap" in the spectrum?