Jianzhong Gu

Density dependence of the nuclear symmetry energy constrained by mean-field calculations

We establish a correlation for the symmetry energy at saturation density

Alpha-decay half-lives and Q_alpha values of superheavy nuclei

S_{0}

Origin of symmetry energy in finite nuclei and density dependence of nuclear matter symmetry energy from measured

, slope parameter

\alpha

L

-decay energies

and curvature parameter

Effects of tensor interaction on pseudospin energy splitting and shell correction

K_{\text{sym}}

Correlation between muonic levels and nuclear structure in muonic atoms

based on widely different mean field interactions. With the help of this correlation and available empirical and theoretical information, the density dependent behavior around the saturation density is determined. We compare the results obtained with the present approach with those by other analyses. With this obtained density dependent behavior of the symmetry energy, the neutron skin thickness of

First-Order Symmetry Energy Induced by Neutron—Proton Mass Difference*

^{208}

Constraints on neutron skin thickness in Pb-208 and density-dependent symmetry energy

Pb and some properties of neutron stars are investigated. In addition, it is found that the expression

Stellar structure of magnetars

S(\rho)=S_{0}(\rho /\rho_{0})^{\gamma}