Effects of the density dependence of nuclear symmetry energy on properties of superheavy nuclei

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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20 pages, 11 figures

Scientific paper

10.1103/PhysRevC.81.044306

Effects of the density dependence of the nuclear symmetry energy on ground-state properties of superheavy nuclei are studied in the relativistic mean-field theory. It is found that the softening of the symmetry energy plays an important role in the empirical shift [Phys. Rev. C 67, 024309 (2003)] of spherical orbitals in superheavy nuclei. The calculation based on the relativistic mean-field models NL3 and FSUGold supports the double shell closure in $^{292}120$ with the softening of the symmetry energy. In addition, the significant effect of the density dependence of the symmetry energy on the neutron skin thickness in superheavy nuclei are investigated.

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