Abstract
In view of new data on the {sup 10}C superallowed Fermi {beta} decay, the radiative corrections have been reevaluated. In particular we calculate and include the nuclear-structure-dependent part of the axial-vector-induced contribution to the {ital O}({alpha}) radiative correction. The resulting {ital V}{sub {ital u}{ital d}} is appreciably larger than a value recently published, which was based on the same data.
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