Neutron skins of heavy nuclei and tidal deformability of neutron star
Abstract
In this paper, I have discussed the numerical predictions for the neutron-skin thickness (NST) of various finite nuclei starting from 40Ca to 238U using recently developed effective relativistic mean-field models G3 and IOPB-I G3, IOPB. The calculated results are compared with the PREX-II data, and the experiment has been done with antiprotons at CERN. Further, I have also calculated the dimensional tidal deformability of a canonical neutron star 1.4M and compared it with the recent observation of GW1701817.
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