2023-02-03 11:30  P5A-1/Online

f-mode imprint in coalescing binaries involving a rapidly rotating neutron star

Dr. Hao-Jui Kuan

The morphology of gravitational waveforms depends on almost all source parameters, and thus encodes a bunch of information about the radiating objects. In particular, tidal parameters of neutron stars may stringently constrain the nuclear equation of state, thus their precise estimation is of fundamental importance. Emphasizing the tidal phase shift by aligned, rotating stars, we provide an accurate, yet economical, method to generate