Abstract
We have reported a systematic shell model description of the experimental Gamow-Teller transition strength for Sc Ca, Ti Sc, Ti V, Co Ni, and Fe Co transitions using KB3G and GXPF1A interactions for model space. In order to see the importance of higher orbital for Co Ni and Fe Co transitions, we have reported the shell model results with space using GXPF1Br+ interaction. We have obtained the qualitative agreement for the individual transitions, while the calculated summed transition strengths closely reproduce the observed ones.
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