Mirror nuclei constraint in nuclear mass formula

Ning Wang, Zuoying Liang, Min Liu, and Xizhen Wu
Phys. Rev. C 82, 044304 – Published 6 October 2010

Abstract

The macroscopic-microscopic mass formula is further improved by considering mirror nuclei constraint. The rms deviation with respect to 2149 measured nuclear masses is reduced to 0.441 MeV. The shell corrections, the deformations of nuclei, the neutron and proton drip lines, and the shell gaps are also investigated to test the model. The rms deviation of α-decay energies of 46 superheavy nuclei is reduced to 0.263 MeV. The predicted central position of the superheavy island could lie around N=176~178 and Z=116~120 according to the shell corrections of nuclei.

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  • Received 4 August 2010

DOI:https://doi.org/10.1103/PhysRevC.82.044304

©2010 American Physical Society

Authors & Affiliations

Ning Wang1,*, Zuoying Liang1, Min Liu1,2, and Xizhen Wu3

  • 1Department of Physics, Guangxi Normal University, Guilin 541004, People’s Republic of China
  • 2College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, People’s Republic of China
  • 3China Institute of Atomic Energy, Beijing 102413, People’s Republic of China

  • *wangning@gxnu.edu.cn

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Vol. 82, Iss. 4 — October 2010

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