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arXiv:1505.01563·v1·Nuclear Theory

Symmetry energy at subsaturation densities and the neutron skin thickness of 208Pb

Xiaohua Fan · Jianmin Dong · Wei Zuo

Abstract

The mass-dependent symmetry energy coefficients has been extracted by analysing the heavy nuclear mass differences reducing the uncertainties as far as possible in our previous work. Taking advantage of the obtained symmetry energy coefficient and the density profiles obtained by switching off the Coulomb interaction in , we calculated the slope parameter of the symmetry energy at the density of . The calculated ranges from 40.5 MeV to 60.3 MeV. The slope parameter of the symmetry energy at the density of is also calculated directly with Skyrme interactions for nuclear matter and is found to have a fine linear relation with the neutron skin thickness of , which is the difference of the neutron and proton rms radii of the nucleus. With the linear relation the neutron skin thickness of is predicted to be 0.15 - 0.21 fm.

Comments: 5 pages, 2 figures

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