A modified effective-range theory (MERT) was introduced previously to describe the scattering of a charged particle by a neutral polarizable system. The long-range components of the resultant effective one-body (generalized optical-model) potential, which cause the phase shift to have a rapidly varying energy dependence, are taken account of exactly by solving a one-body problem numerically. The short-range potential components generate only a slowly varying energy-dependent effect on the phase shift, and this effect can be accounted for by a few terms in a power series in ${k}^{2}$. The procedure is here extended to the case for which the polarizable system is itself charged. An MERT expansion is derived for the difference $\ensuremath{\delta}(k)$ between the total phase shift $\ensuremath{\eta}(k)$ and the phase shift $\ensuremath{\rho}(k)$ due to the long-range tail alone; both $\ensuremath{\eta}(k)$ and $\ensuremath{\rho}(k)$ are defined relative to pure Coulomb scattering. With the strongly energy-dependent Coulombic and other long-range effects accounted for exactly by the numerical solution of a one-body scattering problem, low-energy scattering data can be matched by the proper choice of the coefficients of just the first few terms in the MERT expansion; these terms will then determine the scattering in the (experimentally inaccessible) energy domain extending down to zero energy. For a repulsive Coulomb field, the leading term in $\ensuremath{\eta}(k)$ is determined exactly for all $L$ by the Born approximation; for $V(r)=(\frac{2\ensuremath{\mu}}{{\ensuremath{\hbar}}^{2}})(\ensuremath{-}\frac{{\ensuremath{\beta}}^{2}}{{r}^{4}})$, where $\ensuremath{\alpha}=\frac{{\ensuremath{\beta}}^{2}{\ensuremath{\hbar}}^{2}}{|\ensuremath{\mu}{e}^{2}{Z}_{1}{Z}_{2}}|={\ensuremath{\beta}}^{2}{a}_{0}$ is the electric-dipole polarizability of the target, $tan\ensuremath{\eta}(k)=\frac{{\ensuremath{\beta}}^{2}{{a}_{0}}^{3}{k}^{5}}{15}$ for $k{a}_{0}L\ensuremath{\ll}1$.
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