Abstract
Accurate knowledge about the neutron skin thickness in has far-reaching implications for different communities of nuclear physics and astrophysics. Yet, the novel lead radius experiment (PREX) did not yield any stringent constraint on recently. We employ a more practicable strategy to probe the neutron skin thickness of based on a high linear correlation between the and , where and are the symmetry energy (coefficient) of nuclear matter at saturation density and of . An accurate thus places a strong constraint on the . Compared with the parity-violating asymmetry in the PREX, the reliably experimental information on the is much more easily available thanks to the wealth of measured data on nuclear masses and decay energies. The density dependence of the symmetry energy is also well constrained with the . Finally, with a “tomoscan” method, we find that one just needs to measure the nucleon densities in starting from fm to obtain the in hadron scattering experiments, regardless of its interior profile being hampered by strong absorption.
- Received 9 April 2014
DOI:https://doi.org/10.1103/PhysRevC.91.034315
©2015 American Physical Society