2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/100351Cold atom traps and certain neutron star layers may contain fermions with separation much larger than the range of pair-wise potentials yet much shorter than the scattering length. Such systems can display {\em universal} characteristics independent of the details of the short range interactions. In particular, the energy per particle is a fraction $ξ$ of the Fermi energy of the free Fermion system. Our main result is that for space dimensions D smaller than two and larger than four a specific extension of this problem readily yields $ξ=1$ for all $D \le 2$ whereas $ξ$ is rigorously non-positive (and potentially vanishing) for all $ D \ge 4$. We discuss the D=3 case. A particular unjustified recipe suggests $ξ=1/2$ in D=3.9 pages, 1 figureStrongly Correlated ElectronsOther Condensed MatterMathematical Physicstext