We present a comprehensive investigation of electron capture (EC) ratios
spanning a broad range of atomic numbers. The study employs a self-consistent
computational method that incorporates electron screening, electron
correlations, overlap and exchange corrections, as well as shake-up and
shake-off atomic effects. The electronic wave functions are computed with the
Dirac-Hartree-Fock-Slater (DHFS) method, chosen following a systematic
comparison of binding energies, atomic relaxation energies and Coulomb
amplitudes against other existing methods and experimental data. A novel
feature in the calculations is the use of an energy balance employing atomic
masses, which avoids approximating the electron total binding energy and allows
a more precise determination of the neutrino energy. This leads to a better
agreement of our predictions for capture ratios in comparison with the
experimental ones, especially for low-energy transitions. We expand the
assessment of EC observables uncertainties by incorporating atomic relaxation
energy uncertainties, in contrast to previous studies focusing only on Q-value
and nuclear level energies. Detailed results are presented for nuclei of
practical interest in both nuclear medicine and exotic physics searches
involving liquid Xenon detectors (67Ga, 111In,
123I, 125I and 125Xe). Our study can
be relevant for astrophysical, nuclear, and medical applications.Comment: 16 pages, 9 figures, 4 table