Nuclear symmetry energy probed by neutron skin thickness of nuclei
arXiv:0806.2886 · doi:10.1103/PhysRevLett.102.122502
Abstract
We describe a relation between the symmetry energy coefficients c_sym(rho) of nuclear matter and a_sym(A) of finite nuclei that accommodates other correlations of nuclear properties with the low-density behavior of c_sym(rho). Here we take advantage of this relation to explore the prospects for constraining c_sym(rho) of systematic measurements of neutron skin sizes across the mass table, using as example present data from antiprotonic atoms. The found constraints from neutron skins are in harmony with the recent determinations from reactions and giant resonances.
4 pages, 3 figures, changed content, to appear in Phys. Rev. Lett
References in corpus (7)
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Neutron-Rich Nuclei in Heaven and Earth
- The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
- Isotopic dependence of the giant monopole resonance in the even-A ^{112-124}Sn isotopes and the asymmetry term in nuclear incompressibility
- Neutron and Proton Transverse Emission Ratio Measurements and the Density Dependence of the Asymmetry Term of the Nuclear Equation of State
- Spin-isospin resonances: A self-consistent covariant description
- Why is Tin so soft?
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