An improved calculation of the isospin-symmetry-breaking corrections to superallowed Fermi beta decay

dc.creatorTowner, I. S.
dc.creatorHardy, J. C.
dc.date2007-10-16
dc.date.accessioned2026-07-07T11:12:18Z
dc.date.available2026-07-07T11:12:18Z
dc.descriptionWe report new shell-model calculations of the isospin-symmetry-breaking correction to superallowed nuclear beta decay. The most important improvement is the inclusion of core orbitals, which are demonstrated to have a significant impact on the mismatch in the radial wave functions of the parent and daughter states. We determine which core orbitals are important to include from an examination of measured spectroscopic factors in single-nucleon pick-up reactions. We also examine the new radiative-correction calculation by Marciano and Sirlin and, by a simple reorganization, show that it is possible to preserve the conventional separation into a nucleus-independent inner radiative term and a nucleus-dependent outer term. We tabulate new values for the three theoretical corrections for twenty superallowed transitions, including the thirteen well-studied cases. With these new correction terms the corrected Ft values for the thirteen cases are statistically consistent with one another and the anomalousness of the 46V result disappears. These new calculations lead to a lower average Ft value and a higher value of Vud. The sum of squares of the top-row elements of the CKM matrix now agrees exactly with unitarity.
dc.description15 pages, 2 postscript figures, revtex4
dc.identifierhttps://arxiv.org/abs/0710.3181
dc.identifierhttp://arxiv.org/abs/0710.3181
dc.identifierPhys.Rev.C77:025501,2008
dc.identifierdoi:10.1103/PhysRevC.77.025501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191340
dc.subjectNuclear Theory
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Experiment
dc.titleAn improved calculation of the isospin-symmetry-breaking corrections to superallowed Fermi beta decay
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