Systematic study of bubble nuclei in relativistic mean field model


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We have theoretically studied potential bubble nuclei (20,22O, 34,36Si, and 46Ar), 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, 22Oand 34Si 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.

作者简介

A. Shukla

Rajiv Gandhi Institute of Petroleum Technology

编辑信件的主要联系方式.
Email: amritanshu.shukla@gmail.com
印度, Newdelhi

S. Åberg

Mathematical Physics Division

Email: amritanshu.shukla@gmail.com
瑞典, Stockholm

A. Bajpeyi

Rajiv Gandhi Institute of Petroleum Technology

Email: amritanshu.shukla@gmail.com
印度, Newdelhi

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