Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

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A. Nagar, G. Pratten, G. Riemenschneider, and R. Gamba, A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries, (2019b), arXiv:1904.09550 [gr-qc]

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R. Cotesta, A. Buonanno, A. Bohé, A. Taracchini, I. Hinder, and S. Ossokine, Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics, Phys. Rev. D98

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F. Messina, A. Maldarella, and A. Nagar, Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. II: the higher multipolar modes, Phys. Rev. D97

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A. Nagar et al. , Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects, Phys. Rev. D98

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