Abstract
It is shown that in the central-field approximation, a relativistic calculation reproduces the inverted fine structures experimentally observed in the series of excited sodium nd(3n16) and cesium nf(4n12) terms. Theoretical results are in good agreement with measured values. In view of the simplicity of the method used, it can easily be applied to all the states of a given Rydberg series. This work brings to light the fact that a complete relativistic treatment (which introduces automatically the relativistic contributions on the large components of the wave functions) is equivalent to a multiconfigurational expansion of nonrelativistic wave functions taking into account relativistic corrections (in the low-Z Pauli limit).