 Mass-anisotropy enhancement of a weak-coupling BCS gap

For a fixed-density balanced two-spin Fermi gas with masses $(m,m,\gamma m)$, the Fermi energy scales as ${\gamma }^{-1/3}$ while the single-spin Fermi-level density of states scales as ${\gamma }^{1/3}$. A constant attractive interaction $g$ within a narrow symmetric energy window ${\epsilon }_c\ll {\epsilon }_F$ therefore gives $1={\lambda }_0{\gamma }^{1/3}\mathrm{arsinh}({\epsilon }_c/\Delta )$. Solving gives $\Delta ={\epsilon }_c/\sinh [1/({\lambda }_0{\gamma }^{1/3})]$, whose weak-coupling limit is displayed. Extrapolating to arbitrarily large anisotropy violates the assumptions that the Fermi energy dominates the window and that the pairing coupling is small.