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arxiv: 1407.8054 · v2 · pith:GP3OIZ5Pnew · submitted 2014-07-30 · ⚛️ nucl-th · astro-ph.SR· nucl-ex

Constraining the density slope of nuclear symmetry energy at subsaturation densities using electric dipole polarizability in ²⁰⁸Pb

classification ⚛️ nucl-th astro-ph.SRnucl-ex
keywords textdensityenergynuclearsubsaturationsymmetryalphaconstraint
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Nuclear structure observables usually most effectively probe the properties of nuclear matter at subsaturation densities rather than at saturation density. We demonstrate that the electric dipole polarizibility $\alpha _ {\text{D}}$ in $^{208}$Pb is sensitive to both the magnitude $E_{\text{sym}}(\rho_{\text{c}})$ and density slope $L(\rho_{\text{c}})$ of the symmetry energy at a subsaturation cross density $\rho_{\text{c}} = 0.11$ fm$^{-3}$. Using the experimental data of $\alpha _ {\text{D}}$ in $^{208}$Pb from RCNP and the recent accurate constraint of $E_{\text{sym}}(\rho_{\text{c}})$ from the binding energy difference of heavy isotope pairs, we extract a value of $L(\rho_{\text{c}}) = 47.3 \pm 7.8$ MeV. The implication of the present constraint of $L(\rho_{\text{c}})$ to the symmetry energy at saturation density, the neutron skin thickness of $^{208}$Pb and the core-crust transition density in neutron stars is discussed.

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