Deformed bubble nuclei in the light-mass region
Nuclei with a central region of low nucleonic density, "bubble" nuclei, are studied. In particular, the possibility of bubbles in deformed nuclei is discussed, concentrating on experimentally accessible light nuclei. Utilizing the relativistic mean field (RMF) model we find favorable candidates in the prolately deformed Ne-24 nucleus and the mirror nuclei Si-32 and Ar-32 with oblate shapes.