Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach
Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach
Extracting the unique information on ultradense nuclear matter from the gravitational waves emitted by merging neutron-star binaries requires robust theoretical models of the signal. We develop a novel effective-one-body waveform model that includes, for the first time, dynamic (instead of only adiabatic) tides of the neutron star as well as …