Note on neutron star equation of state in the light of GW170817
Note on neutron star equation of state in the light of GW170817
From the very first multimessenger event of GW170817, clean robust constraints can be obtained for the tidal deformabilities of the two stars involved in the merger, which provides us unique opportunity to study the equation of states (EOSs) of dense stellar matter. In this contribution, we employ a model from …