Abstract
Numerical solutions of the Schrödinger equation with the complete screened Coulomb potential (CSCP) are given for 1s, 2s, 2p, 3s, 3p, and 3d states. The CSCP used is given by {V(r)=,Vi(r)Ze2[r1(D+A)1],  0rA}{=V0(r)Ze2[D(D+A)]{exp[(Ar)D]r},  rA} where D is the screening radius and A is the mean minimum radius of the ion atmosphere. The standard transformations x=2Zrλa0 and Eλ=Z2μe422λ2, where λ is the CSCP quantum number, yield the well-known form of the Schrödinger equation with λ in place of n. The numerical solutions are obtained with a nonlinear method that is both accurate and stable. The resulting quantum numbers can be accurately described by simple analytic fits for a wide range of interesting values of D. The problem of the number of screened Coulomb states is resolved: the CSCP yields as many states as the Coulomb potential. However, with the CSCP, for states with (3a0n22Z)>D, the separations of the levels are less than the corresponding Coulomb levels, i.e., the density of states near the continuum increases. Removal of l-degeneracy, the question of a maximum-bound principal quantum number, and integer quantization of the ground-state quantum numbers are also discussed.