Abstract
Under the assumption that isospin is a good quantum number, isobaric analog states and various analogous transitions are expected in isobars with mass number . The strengths of analogous Gamow-Teller (GT) transitions and analogous transitions within the isobar quartet are compared in detail. The GT transitions from the ground state of leading to excited , , and states in were measured using the charge-exchange reaction. With a high energy resolution of , many fragmented states were observed, and the GT strength distribution was determined up to excitation energy . The main part of the strength was concentrated in the region. A shell-model calculation could reproduce the concentration, but not so well details of the strength distribution. The obtained distribution was further compared with two results of decay studying the analogous GT strengths. They reported contradicting distributions. One-to-one correspondences of analogous transitions and analog states were assigned up to in the comparison with one of these -decay results. Combining the spectroscopic information of the analog states in and , the most probable values were deduced for each pair of analog states. It was found that states carry the main part of the observed GT strength, while much less GT strength was carried by and states. The gross features of the GT strength distributions for each were similar for the isospin analogous transitions, but the details were somewhat different. From the difference of the distributions, isospin-asymmetry matrix elements of were deduced. The Coulomb displacement energy, which is sensitive to the configuration of states, showed a sudden increase of about at the excitation energy of . The strengths of several transitions to the IAS in were compared with the strengths of analogous GT transitions. It was found that ratios of the and GT transition strengths were similar, suggesting that the contributions of the term in transitions are small.
1 More- Received 31 July 2004
DOI:https://doi.org/10.1103/PhysRevC.70.054311
©2004 American Physical Society