Quantitative predictions for atomic-electron screening effects in low-energy pair production follow from the knowledge that the small-distance shape of screened-electron and positron continuum wave functions is close to that of point-Coulomb wave functions of shifted energy. These predictions are verified by making exact numerical calculations in representative cases. The energy-shift normalization theory is then used in conjunction with the point-Coulomb results of @verb/ to obtain predictions for atomic-pair-production energy distributions and total cross sections for photon energies from threshold to 5 MeV. Atomicelectron screening effects cause appreciable modifications of the total cross sections for photon energies below 1.5 MeV and continue to have a major effect on some portions of the energy distribution at higher photon energies. Results are also compared with Bethe-Heitler predictions and with experiments.With the continuing improvements in computers it is becoming feasible to make fairly accurate theoretical calculations of atomic-pair-production cross sections in the low-energy region where the Bethe-Maximon~high-energy results and Born approximation (the well-known Bethe -Heitler formula) need not be valid. Relativistic calculations of pair production in a point-Coulomb-potential model have now been reported by Qhrerbg Mork, and Olsen (QlMO); more extensive results have been given by (|)verbg'. This use of a point-Coulomb model relies on the expectation, based on form-factor estimates, 4 that the effects of atomic-electron screening would be unimportant in this energy region. Such an estimate is obtained because the maximum impact parameter r~discussed by Heitler, 5 equal to q~, with q &, = k' -P, p, is of the order of the electron Compton wavelength and is quite small compared to the radius of the atom. However, we subsequently performed the lengthy relativistic calculations~of pair-production cross sections in screened potentials and found that, near threshold, atomic-electron screening effects are important. At electron-Comptonwavelength distances an electron sees a point-Coulomb potential corresponding to the nuclear charge Z. The electron wave function has a hydrogenlike shape; the only effect of atomic-electron screening, as described by a central potential V deviating from the point-Coulomb form, is to modify the normalization.For a very-low-energy continuum wave function (but not for higher energies) this normalization is indeed sensitive to the screening. We showed in fact that we could roughly obtain screened pair-production cross sections from point-Coulomb cross sections simply by using a multiplicative normalization factor.We have recently examined~in greater detail the