Higher-order corrections to the field shift in atomic systems
arXiv:2607.26902
The paper develops a systematic expansion for higher-order contributions to the field shift in atomic spectra, validates it with numerical calculations for hydrogen-like ions, and extends the analysis to alkali-like ions, showing that these corrections have a nearly charge‑independent ratio and do not affect King‑plot linearity under a certain approximation.
Abstract
Differences in nuclear charge distributions between isotopes lead to small changes in atomic spectra known as the field shift. While largely proportional to the change in the mean-square nuclear radius, the field shift also contains higher-order contributions with different dependencies on nuclear moments. Their knowledge is required in searches for new physics using King plots, as they can induce deviations from King-plot linearity. We present a systematic expansion of the field-shift energies in terms of nuclear parameters and test its validity against direct numerical calculations for H-like ions. We also compute leading- and higher-order field-shift corrections for alkali-like systems from Li-like to Rb-like ions, and find that their ratio is nearly independent of the ionic charge state, agreeing with the corresponding hydrogenic ratios on a sub-percent level. Motivated by this observation, we introduce an approximation in which these fractional contributions are assumed to be independent of the electronic configuration. We show that within this approximation, higher-order field-shift corrections do not contribute to King-plot nonlinearities.