no code implementations • 14 Jan 2021 • Xuhao Wu, Shishao Bao, Hong Shen, Renxin Xu
The constraints from the mass of 2. 6 $M_{\odot}$ and the tidal deformability $\Lambda_{1. 4}=616_{-158}^{+273}$ (based on the assumption that GW190814 is a neutron star-black hole binary) can be satisfied as the slope of symmetry energy $L \leq 50$ MeV.
Nuclear Theory High Energy Astrophysical Phenomena
