Abstract
Background: Aspects of the nuclear structure of light -conjugate nuclei have long been associated with nuclear clustering based on particles and heavier -conjugate systems such as and . Such structures are associated with strong deformation corresponding to superdeformed or even hyperdeformed bands. Superdeformed bands have been identified in and neighboring nuclei and find good description within shell model, mean-field, and -cluster models. The utility of the -cluster description may be probed further by extending such studies to more challenging cases comprising lighter -conjugate nuclei such as , and .
Purpose: The purpose of this study is to look for the number and energy of isoscalar states in . These states are the potential bandheads for superdeformed bands in corresponding to the exotic structures of . Of particular interest is locating the bandhead of the previously identified superdeformed band in .
Methods: -particle inelastic scattering from a target at very forward angles including has been performed at the iThemba Laboratory for Accelerator-Based Sciences in South Africa. Scattered particles corresponding to the excitation energy region of 6 to 14 MeV were momentum-analysed in the K600 magnetic spectrometer and detected at the focal plane using two multiwire drift chambers and two plastic scintillators.
Results: Several states have been identified above 9 MeV in . A newly identified 9.71 MeV state is a strong candidate for the bandhead of the previously discussed superdeformed band. The multichannel dynamical symmetry of the semimicroscopic algebraic model predicts the spectrum of the excited states. The theoretical prediction is in good agreement with the experimental finding, supporting the assignment of the 9.71-MeV state as the bandhead of a superdeformed band.
Conclusion: Excited isoscalar states in have been identified. The number of states observed in the present experiment shows good agreement with the prediction of the multichannel dynamical symmetry.
- Received 5 September 2016
DOI:https://doi.org/10.1103/PhysRevC.95.024319
©2017 American Physical Society