Multicluster configuration in highly excited states of 24Mg

M. Ito, Y. Hirabayashi, and Y. Sakuragi
Phys. Rev. C 66, 034307 – Published 6 September 2002
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Abstract

The nuclear structure of 24Mg with 12C+3α and 3α+3α configurations, existing at an extremely highly-excited energy domain is studied by the microscopic coupled-channels (MCC) calculation based on the double-folding interactions using 3α-RGM wave functions of 12C and a realistic nucleon-nucleon interaction called DDM3Y. The dinuclear 12C+12C configuration of 24Mg, corresponding to the so-called “higher-energy molecular resonances,” is also investigated by the same MCC framework. The MCC calculation predicts the existence of three kinds of the molecular bands having 3α+3α, 12C+3α, and 12C+12C structures around the excitation energy of about 40 MeV with respect to the ground state of 24Mg. The channel coupling among the 3α states in each 12C plays very important roles for the formation of the 12C+3α and 3α+3α molecular bands. It is found that the populations of the 12Cg.s.+12Cg.s., 12Cg.s.+12C(02+), and 12C(02+)+12C(02+) channels are very small in the individual molecular bands with 12C+12C, 12C+3α, and 3α+3α configurations, respectively. The reaction mechanism for the inelastic scattering leading to the 12Cg.s.+12C(02+) and 12C(02+)+12C(02+) excitation channels is also investigated in relation to the obtained three kinds of the molecular bands. The result suggests that the inelastic scattering to the 12C(02+)+12C(02+) [12Cg.s.+12C(02+)] channel can be interpreted in terms of weak transitions from the 12Cg.s.+12Cg.s. component of the 12C+12C molecular bands to the 12C(02+)+12C(02+) [12Cg.s.+12C(02+)] component of the multicluster 3α+3α (12C+3α) molecular bands. All the results are discussed in connection with the band crossing model which was proposed in describing the higher-energy molecular resonance with dinuclear configuration as well as the resonances observed in the 12C(02+)+12C(02+) and 12Cg.s.+12C(02+) exit channels.

  • Received 9 May 2002

DOI:https://doi.org/10.1103/PhysRevC.66.034307

©2002 American Physical Society

Authors & Affiliations

M. Ito1, Y. Hirabayashi2, and Y. Sakuragi3

  • 1Division of Physics, Graduate School of Science, Hokkaido University, Sapporo 060-0810, Japan
  • 2Center for Information and Multimedia Studies, Hokkaido University, Sapporo 060-0811, Japan
  • 3Department of Physics, Osaka City University, Osaka 558-8585, Japan

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Vol. 66, Iss. 3 — September 2002

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