We have theoretically studied potential bubble nuclei (O-20,O-22, Si-34,Si-36, and Ar-46), which are experimentally accessible and have attracted several studies in the recent past. Relativistic mean field is employed in conjunction with the NL-SH parameter set. Our results show that among the possible candidates, O-22 and Si-34 may be the most prominent candidates, showing significant depletion of density at the center, which could be verified experimentally in the near future with some of the experiments underway.
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