Merger of binary neutron stars with realistic equations of state in full general relativity
Merger of binary neutron stars with realistic equations of state in full general relativity
We present numerical results of three-dimensional simulations for the merger of binary neutron stars (BNSs) in full general relativity. Hybrid equations of state (EOSs) are adopted to mimic realistic nuclear EOSs. In this approach, we divide the EOSs into two parts, i.e., the thermal part and the cold part. For …