Consistent relativistic mean-field models constrained by GW170817

We have obtained the Love number and corresponding tidal deformabilities () associated with the relativistic mean-field parametrizations shown to be consistent (CRMF) with the nuclear matter, pure neutron matter, symmetry energy, and its derivatives Dutra et al. , Phys. Rev. C 90, 055203 (2014). Our results show that CRMF models present very good agreement with the recent data from binary neutron star merger event GW170817. They also confirm the strong correlation between ₁. ₄ and the radius of canonical stars (R₁. ₄). When a recent GW170817 constraint on ₁. ₄ and the corresponding radius R₁. ₄ is used, the majority of the models tested are shown to satisfy it.