New and robust gravitational-waveform model for high-mass-ratio binary neutron star systems with dynamical tidal effects
New and robust gravitational-waveform model for high-mass-ratio binary neutron star systems with dynamical tidal effects
For the analysis of gravitational-wave signals, fast and accurate gravitational-waveform models are required. These enable us to obtain information on the system properties from compact binary mergers. In this article, we introduce the model, which contains a closed-form expression that describes tidal effects, focusing on the description of binary neutron …