Abstract
We study Gamow–Teller strength distributions in some selected nuclei of particular astrophysical interest within the iron mass region. The theoretical framework is based on a proton–neutron quasiparticle random phase approximation built on a deformed selfconsistent mean field basis obtained from two-body density-dependent Skyrme forces. We compare our results to available experimental information obtained from ( n, p) and ( p, n) charge exchange reactions.
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