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Turkish Journal of Physics

Authors

WALEED HWASH

DOI

10.3906/fiz-1611-18

Abstract

The microscopic cluster model approach has been performed to study the nuclear structure of the lightest and heaviest two-neutron halo nuclei, $^{6}$He and $^{22}$C, respectively. The matter radius and binding energy for the $^{6}$He and $^{22}$C nuclei are calculated and the effect of the core deformation ($^{20}$C) on the properties of $^{22}$C nuclei is also discussed. Calculations have shown that the microscopic cluster model provides a good description of binding energy as well as matter radius in comparison to experimental data. The fittings of some parameters such as central potential depth (V$_{o})$, empirical constant (r$_{o})$, and surface diffuseness value (a) are discussed to find agreement in the results with the available experimental data. The exotic properties of two-neutron halo nuclides $^{6}$He and $^{22}$C such as weak binding energy, abnormal large matter radius, and Borromean system have been confirmed in the present work.

Keywords

Halo nuclei, cluster model, nuclear structure, exotic nuclei

First Page

151

Last Page

159

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