Strong Post-merger Gravitational Radiation of GW170817-like Events
Strong Post-merger Gravitational Radiation of GW170817-like Events
The post-merger gravitational wave (GW) radiation of the remnant formed in the binary neutron star (BNS) coalescence has not been directly measured, yet. We show in this work that the properties of the BNS involved in GW170817, additionally constrained by PSR J0030+0451, the lower limit on the maximum gravitational mass …