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Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects

Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects

The combined observation of gravitational and electromagnetic waves from the coalescence of two neutron stars marks the beginning of multi-messenger astronomy with gravitational waves (GWs). The development of accurate gravitational waveform models is a crucial prerequisite to extract information about the properties of the binary system that generated a detected …