The response of the nuclear energy to changes in neutron and proton surface
diffusenesses is investigated using the Thomas-Fermi model. Algebraic expr
essions are provided for the energy cost of changing the two diffusenesses
away from their equilibrium values. This will make it possible to generaliz
e the macroscopic-microscopic calculations of nuclear masses and deformatio
n energies by the inclusion of the neutron and proton diffusenesses as degr
ees of freedom (to be varied along with the shape degrees of freedom). One
result, which is suggested by the relatively low cost in macroscopic energy
of increasing the diffuseness of a heavy nucleus by 10% (abour 4 MeV), is
that superheavy nuclei near Z=126, N=184 may have a fair chance of becoming
stabilized by shell effects. An appendix introduces an improved measure of
surface diffuseness, with certain advantages over the conventional Sussman
n width b. [S0556-2813(98)03612-7].