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Gamow-Teller transitions and magnetic properties of nuclei and shell evolution

Toshio Suzuki*

Rintaro Fujimoto

Takaharu Otsuka

  • Department of Physics, College of Humanities and Sciences, Nihon University, Sakurajosui 3-25-40, Setagaya-ku, Tokyo 156, Japan

  • Department of Physics, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

  • Department of Physics and Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
  • RIKEN, Hirosawa, Wako-shi, Saitama 351-0198, Japan

  • *Email address: suzuki@chs.nihon-u.ac.jp

Phys. Rev. C 67, 044302 – Published 18 April, 2003

DOI: https://doi.org/10.1103/PhysRevC.67.044302

Abstract

New aspects of quenching of Gamow-Teller (GT) transitions and magnetic moments are investigated for p-shell nuclei using an improved shell-model Hamiltonian with enhanced spin-flip proton-neutron interaction and modified single-particle energies. The present shell-model Hamiltonian thus obtained is used in the configuration space up to (2–3)ħω excitations, and GT transitions and magnetic moments are calculated with bare g factors and bare axial-vector coupling constant. Manifestation of variable quenching due to changing gap between 0p3/2 and 0p1/2 is presented in GT transitions such as 12C12N, 11B11Be, and 9Li9Be. A similar effect is shown for magnetic moments. Better agreement with experimental values is obtained systematically by using the present Hamiltonian for GT transitions and magnetic moments in most of p-shell nuclei, as well as for energy levels. Thus, the shell structure is changing from nucleus to nucleus in an orderly way (i.e., shell evolution), the inclusion of which leads us to an improved description of the GT and magnetic properties. It is stressed that the anomalous shell structure of exotic nuclei and the GT/magnetic properties of stable and exotic nuclei are linked through the same underlying mechanism.

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