The authors find that reproducing a 2.1 solar mass maximum neutron star requires a neutron effective mass of 0.60-0.65 at saturation density, leading to radius 12.4 km and tidal deformability 423 for a 1.4 solar mass star.
Extremes of Density and 5 Temperature: Cosmic Matter in the Laboratory
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Constraints on Skyrme Equations of State from Doubly Magic Nuclei, Ab-Initio Calculations of Low-Density Neutron Matter, and Neutron Stars
The authors find that reproducing a 2.1 solar mass maximum neutron star requires a neutron effective mass of 0.60-0.65 at saturation density, leading to radius 12.4 km and tidal deformability 423 for a 1.4 solar mass star.