Self-consistent random phase approximation (RPA) approaches in the
relativistic framework are applied to calculate the isospin symmetry-breaking
corrections δc​ for the 0+→0+ superallowed transitions. It is
found that the corrections δc​ are sensitive to the proper treatments of
the Coulomb mean field, but not so much to specific effective interactions.
With these corrections δc​, the nucleus-independent Ft
values are obtained in combination with the experimental ft values in the
most recent survey and the improved radiative corrections. It is found that the
constancy of the Ft values is satisfied for all effective
interactions employed. Furthermore, the element Vud​ and unitarity of the
Cabibbo-Kobayashi-Maskawa matrix are discussed.Comment: 7 pages, 2 figures, 4 table