Effective-one-body waveform model for non-circularized, planar, coalescing black hole binaries: the importance of radiation reaction

M. Boyle et al. , The SXS Collaboration catalog of binary black hole simulations, Class. Quant. Grav. 36

Original

1904

Earlier work this paper cites.

D. Bini, T. Damour, and A. Geralico, Novel approach to binary dynamics: application to the fifth post-Newtonian level, Phys. Rev. Lett. 123

Original

1909

Earlier work this paper cites.

T. Damour, B. R. Iyer, and B. S. Sathyaprakash, Improved filters for gravitational waves from inspiralling compact binaries, Phys. Rev. D57

1998

Earlier work this paper cites.

A. Buonanno and T. Damour, Effective one-body approach to general relativistic two-body dynamics, Phys. Rev. D59

1999

Earlier work this paper cites.

D. Chiaramello and A. Nagar, Faithful analytical effective-one-body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries, Phys. Rev. D 101

Original

2001

Earlier work this paper cites.

A. Nagar, G. Riemenschneider, G. Pratten, P. Rettegno, and F. Messina, Multipolar effective one body waveform model for spin-aligned black hole binaries, Phys. Rev. D 102

Original

2001

Earlier work this paper cites.

A. Antonelli, C. Kavanagh, M. Khalil, J. Steinhoff, and J. Vines, Gravitational spin-orbit coupling through third-subleading post-Newtonian order: from first-order self-force to arbitrary mass ratios, Phys. Rev. Lett. 125

Original

2003

Earlier work this paper cites.

T. Damour and A. Nagar, Comparing Effective-One-Body gravitational waveforms to accurate numerical data, Phys. Rev. D77

Original

2008

Earlier work this paper cites.

S. Hild, S. Chelkowski, and A. Freise, Pushing towards the ET sensitivity using ’conventional’ technology, (2008), arXiv:0810.0604 [gr-qc]

Original

2008

Earlier work this paper cites.

A. Nagar, P. Rettegno, R. Gamba, and S. Bernuzzi, Effective-one-body waveforms from dynamical captures in black hole binaries, Phys. Rev. D 103

Original

2009

Earlier work this paper cites.

T. Damour and A. Nagar, An improved analytical description of inspiralling and coalescing black-hole binaries, Phys. Rev. D79

Original

2009

Earlier work this paper cites.

V. Gayathri, J. Healy, J. Lange, B. O’Brien, M. Szczepanczyk, I. Bartos, M. Campanelli, S. Klimenko, C. O. Lousto, and R. O’Shaughnessy, Eccentricity estimate for black hole mergers with numerical relativity simulations, Nature Astron. 6

Original

2009

Earlier work this paper cites.

R. Fujita and B. R. Iyer, Spherical harmonic modes of 5.5 post-Newtonian gravitational wave polarizations and associated factorized resummed waveforms for a particle in circular orbit around a Schwarzschild black hol, Phys. Rev. D82

Original

2010

Earlier work this paper cites.

A. Antonelli, C. Kavanagh, M. Khalil, J. Steinhoff, and J. Vines, Gravitational spin-orbit and aligned spin 1 -spin 2 couplings through third-subleading post-Newtonian orders, Phys. Rev. D 102

Original

2010

Earlier work this paper cites.

S. Hild, S. Chelkowski, A. Freise, J. Franc, N. Morgado, R. Flaminio, and R. DeSalvo, A Xylophone Configuration for a third Generation Gravitational Wave Detector, Class. Quant. Grav. 27

Original

2010

Earlier work this paper cites.

S. Hild et al. , Sensitivity Studies for Third-Generation Gravitational Wave Observatories, Class. Quant. Grav. 28

Original

2011

Earlier work this paper cites.

D. Bini and T. Damour, Gravitational radiation reaction along general orbits in the effective one-body formalism, Phys.Rev. D86

Original

2012

Earlier work this paper cites.

A. Taracchini, Y. Pan, A. Buonanno, E. Barausse, M. Boyle, et al. , Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms, Phys.Rev. D86

Original

2012

Earlier work this paper cites.

R. Fujita, Gravitational radiation for extreme mass ratio inspirals to the 14th post-Newtonian order, Prog.Theor.Phys. 127

Original

2012

Earlier work this paper cites.

T. Damour, A. Nagar, and S. Bernuzzi, Improved effective-one-body description of coalescing nonspinning black-hole binaries and its numerical-relativity completion, Phys.Rev. D87

Original

2013

Cited alongside, same era.

T. Damour, F. Guercilena, I. Hinder, S. Hopper, A. Nagar, and L. Rezzolla, Strong-Field Scattering of Two Black Holes: Numerics Versus Analytics, Phys. Rev. D 89

Original

2014

Cited alongside, same era.

G. Faye, L. Blanchet, and B. R. Iyer, Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order, Class. Quant. Grav. 32

Original

2015

Cited alongside, same era.

A. Nagar and A. Shah, Factorization and resummation: A new paradigm to improve gravitational wave amplitudes, Phys. Rev. D94

Original

2016

Cited alongside, same era.

A. Nagar and S. Albanesi, Toward a gravitational self-force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals, Phys. Rev. D 106

Original

2022

Later among the works it cites.

A. M. Knee, I. M. Romero-Shaw, P. D. Lasky, J. McIver, and E. Thrane, A Rosetta Stone for Eccentric Gravitational Waveform Models, Astrophys. J. 936

Original

2022

Later among the works it cites.

A. Bonino, R. Gamba, P. Schmidt, A. Nagar, G. Pratten, M. Breschi, P. Rettegno, and S. Bernuzzi, Inferring eccentricity evolution from observations of coalescing binary black holes, Phys. Rev. D 107

Original

2023

Later among the works it cites.

R. Gamba, M. Breschi, G. Carullo, S. Albanesi, P. Rettegno, S. Bernuzzi, and A. Nagar, GW190521 as a dynamical capture of two nonspinning black holes, Nature Astron. 7

Original

2023

Later among the works it cites.