Citing Articles For: Real modes and null memory contributions in effective-one-body models

Modeling the merger-ringdown of an eccentric test-mass inspiral into a Kerr black hole using the effective-one-body framework

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Ringdown modeling for effective-one-body waveforms in the test-mass limit for eccentric equatorial orbits around a Kerr black hole

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Toward claiming a detection of gravitational memory

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Black-hole–neutron-star mergers: New numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity

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Waveform models for the gravitational-wave memory effect. II. Time-domain and frequency-domain models for nonspinning binaries

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Impact of the (ℓ=2, m=0) spherical harmonic mode with memory on parameter estimation for ground-based detectors

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Perturbative hyperboloidal extraction of gravitational waves in 3+1 numerical relativity

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Waveform model for the (ℓ=2,m=0) spherical harmonic and the displacement memory contribution from precessing binary black holes

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Effective-one-body modeling for generic compact binaries with arbitrary orbits

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Phys. Rev. D 112 L121503 (2025)

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Articles Citing

Real modes and null memory contributions in effective-one-body models

Modeling the merger-ringdown of an eccentric test-mass inspiral into a Kerr black hole using the effective-one-body framework

Ringdown modeling for effective-one-body waveforms in the test-mass limit for eccentric equatorial orbits around a Kerr black hole

Dynamical quasinormal mode excitation

Adding equatorial-asymmetric effects for spin-precessing binaries into the seobnrv5phm waveform model

Toward claiming a detection of gravitational memory

Black-hole–neutron-star mergers: New numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity

Advancing the effective-one-body framework in the test-mass limit

Waveform models for the gravitational-wave memory effect. II. Time-domain and frequency-domain models for nonspinning binaries

Characterizing the merger of equatorial-eccentric-geodesic plunges in rotating black holes

Impact of the (ℓ=2, m=0) spherical harmonic mode with memory on parameter estimation for ground-based detectors

Perturbative hyperboloidal extraction of gravitational waves in 3+1 numerical relativity

Waveform model for the (ℓ=2,m=0) spherical harmonic and the displacement memory contribution from precessing binary black holes

Effective-one-body modeling for generic compact binaries with arbitrary orbits

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