Shrunk halo and quenched shell gap at in C: Inversion of states and deformation effects
arXiv:1807.04991 · doi:10.1016/j.physletb.2018.08.071
Abstract
We investigate the ground state properties of C by using a deformed relativistic Hartree-Bogoliubov model in continuum and explore the interplays among the formation of a halo, deformation effects, the inversion of states, the shell evolution, and changes of nuclear magicities. It is revealed that there is an inversion between the two spherical orbitals and in C compared with the conventional single particle shell structure in stable nuclei. This inversion, together with deformation effects, results in a shrunk halo and a quenched shell gap at . It is predicted that the core of C is oblate but the halo is prolate. Therefore several exotic nuclear phenomena, including the halo, the shape decoupling effects, the inversion of states, and the evolution of shell structure which results in (dis)appearance of magic numbers, coexist in one single nucleus .
arXiv commentPhys. Lett. B, in press
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