Ground-state energies and superfluid gaps are calculated for degenerate Fer
mi systems interacting via long attractive scattering lengths such as cold
atomic gases, neutron, and nuclear matter. In the intermediate region of de
nsities, where the interparticle spacing (similar to1/k(F)) is longer than
the range of the interaction but shorter than the scattering length, the su
perfluid gaps and the energy per particle are found to be proportional to t
he Fermi energy and thus differ from the dilute and high-density limits. Th
e attractive potential increase linearly with the spin-isospin or hyperspin
statistical factor such that, e.g., symmetric nuclear matter undergoes spi
nodal decomposition and collapses whereas neutron matter and Fermionic atom
ic gases with two hyperspin states are mechanically stable in the intermedi
ate density region. The regions of spinodal instabilities in the resulting
phase diagram are reduced and do not prevent a superfluid transition.