The G3 and IOPB-I mean-field parameter sets are used to predict neutron-skin thicknesses for 26 nuclei and the 1.4 solar mass neutron star tidal deformability, with only the G3 value satisfying the tighter GW170817 re-analysis bound.
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Neutron skins of heavy nuclei and tidal deformability of neutron star
The G3 and IOPB-I mean-field parameter sets are used to predict neutron-skin thicknesses for 26 nuclei and the 1.4 solar mass neutron star tidal deformability, with only the G3 value satisfying the tighter GW170817 re-analysis bound.