On the detectability of higher harmonics with LISA

Supermassive black hole binaries (SMBHBs) are expected to be detected by the future space-based gravitational-wave detector LISA with a large signal-to-noise ratio (SNR). This prospect enhances the possibility of differentiating higher harmonics in the inspiral-merger-ringdown (IMR) waveform. In thi...

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Veröffentlicht in:	arXiv.org 2023-07
Hauptverfasser:	Pitte, Chantal, Baghi, Quentin, Marsat, Sylvain, Besançon, Marc, Petiteau, Antoine
Format:	Artikel
Sprache:	eng
Schlagworte:	Bayesian analysis Bias Gravitational waves Higher harmonics Mathematical models Parameter estimation Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Signal to noise ratio Supermassive black holes Waveforms
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