Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms

D. Gerosa, S. Ma, K. W. K. Wong, E. Berti, R. O’Shaughnessy, Y. Chen, and K. Belczynski, Multiband gravitational-wave event rates and stellar physics, Phys. Rev. D 99

Original

1902

Earlier work this paper cites.

B. Moore and N. Yunes, A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity, Class. Quant. Grav. 36

Original

1903

Earlier work this paper cites.

Y. Boetzel, C. K. Mishra, G. Faye, A. Gopakumar, and B. R. Iyer, Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Tail contributions and postadiabatic corrections, Phys. Rev. D 100

Original

1904

Earlier work this paper cites.

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

Original

1904

Earlier work this paper cites.

A. Nagar, G. Pratten, G. Riemenschneider, and R. Gamba, Multipolar effective one body model for nonspinning black hole binaries, Phys. Rev. D 101

Original

1904

Earlier work this paper cites.

M. Ebersold, Y. Boetzel, G. Faye, C. K. Mishra, B. R. Iyer, and P. Jetzer, Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions, Phys. Rev. D 100

Original

1906

Earlier work this paper cites.

D. Reitze et al. , Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO, Bull. Am. Astron. Soc. 51

Original

1907

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.

A. Ramos-Buades, S. Husa, G. Pratten, H. Estellés, C. García-Quirós, M. Mateu-Lucena, M. Colleoni, and R. Jaume, First survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation, Phys. Rev. D 101

Original

1909

Earlier work this paper cites.

U. Sperhake, R. Rosca-Mead, D. Gerosa, and E. Berti, Amplification of superkicks in black-hole binaries through orbital eccentricity, Phys. Rev. D 101

Original

1910

Earlier work this paper cites.

X. Liu, Z. Cao, and L. Shao, Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits, Phys. Rev. D 101

Original

1910

Earlier work this paper cites.

M. Maggiore et al. , Science Case for the Einstein Telescope, JCAP 03

Original

1912

Earlier work this paper cites.

T. Regge and J. A. Wheeler, Stability of a Schwarzschild singularity, Phys. Rev. 108

1957

Earlier work this paper cites.

E. Newman and R. Penrose, An Approach to gravitational radiation by a method of spin coefficients, J. Math. Phys. 3

1962

Earlier work this paper cites.

P. C. Peters and J. Mathews, Gravitational radiation from point masses in a Keplerian orbit, Phys. Rev. 131

1963

Earlier work this paper cites.

P. C. Peters, Gravitational Radiation and the Motion of Two Point Masses, Phys. Rev. 136

1964

Earlier work this paper cites.

D. Christodoulou, Reversible and irreversible transforations in black hole physics, Phys. Rev. Lett. 25

1970

Earlier work this paper cites.

F. J. Zerilli, Effective potential for even parity Regge-Wheeler gravitational perturbation equations, Phys. Rev. Lett. 24

1970

Earlier work this paper cites.

H. O. Kreiss and J. Oliger, Methods for the approximate solution of time dependent problems (International Council of Scientific Unions, World Meteorological Organization, Geneva, 1973)

1973

Earlier work this paper cites.

J. M. Bowen and J. W. York, Jr., Time asymmetric initial data for black holes and black hole collisions, Phys. Rev. D21

1980

Earlier work this paper cites.

T. Damour and N. Deruelle, General relativistic celestial mechanics of binary systems. I. The post-newtonian motion, Annales de l’I.H.P. Physique théorique 43

1985

Earlier work this paper cites.

T. Damour and G. Schäfer, Higher Order Relativistic Periastron Advances and Binary Pulsars, Nuovo Cim. B101

1988

Earlier work this paper cites.

C. W. Lincoln and C. M. Will, Coalescing binary systems of compact objects to ( post ) 5 / 2 {(\mathrm{post})}^{5/2} -newtonian order: Late-time evolution and gravitational-radiation emission, Phys. Rev. D 42

1990

Earlier work this paper cites.

T. A. Apostolatos, C. Cutler, G. J. Sussman, and K. S. Thorne, Spin induced orbital precession and its modulation of the gravitational wave forms from merging binaries, Phys. Rev. D49

1994

Earlier work this paper cites.

L. E. Kidder, Coalescing binary systems of compact objects to postNewtonian 5/2 order. 5. Spin effects, Phys.Rev. D52

1995

Earlier work this paper cites.

M. Shibata and T. Nakamura, Evolution of three-dimensional gravitational waves: Harmonic slicing case, Phys. Rev. D52

1995

Earlier work this paper cites.

C. Bona, J. Massó, E. Seidel, and J. Stela, New Formalism for Numerical Relativity, Phys. Rev. Lett. 75

1995

Earlier work this paper cites.

S. Brandt and B. Brügmann, A Simple construction of initial data for multiple black holes, Phys. Rev. Lett. 78

1997

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.

T. W. Baumgarte and S. L. Shapiro, On the numerical integration of Einstein’s field equations, Phys. Rev. D59

1999

Earlier work this paper cites.

A. Buonanno and T. Damour, Transition from inspiral to plunge in binary black hole coalescences, Phys. Rev. D62

2000

Earlier work this paper cites.

T. Damour, P. Jaranowski, and G. Schaefer, On the determination of the last stable orbit for circular general relativistic binaries at the third postNewtonian approximation, Phys. Rev. D62

2000

Earlier work this paper cites.

K. Belczynski, V. Kalogera, and T. Bulik, A Comprehensive study of binary compact objects as gravitational wave sources: Evolutionary channels, rates, and physical properties, Astrophys. J. 572

2001

Earlier work this paper cites.

T. Damour, Coalescence of two spinning black holes: An effective one- body approach, Phys. Rev. D64

2001

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. Ramos-Buades, P. Schmidt, G. Pratten, and S. Husa, Validity of common modeling approximations for precessing binary black holes with higher-order modes, Phys. Rev. D 101

Original

2001

Earlier work this paper cites.

O. Sarbach and M. Tiglio, Gauge invariant perturbations of Schwarzschild black holes in horizon-penetrating coordinates, Phys. Rev. D64

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.

T. Mora and C. M. Will, Numerically generated quasiequilibrium orbits of black holes: Circular or eccentric?, Phys. Rev. D 66

2002

Earlier work this paper cites.

D. Bini, T. Damour, and A. Geralico, Binary dynamics at the fifth and fifth-and-a-half post-Newtonian orders, Phys. Rev. D 102

Original

2003

Earlier work this paper cites.

M. Alcubierre, B. Brügmann, P. Diener, M. Koppitz, D. Pollney, et al. , Gauge conditions for long term numerical black hole evolutions without excision, Phys.Rev. D67

2003

Earlier work this paper cites.

A. Ashtekar and B. Krishnan, Dynamical horizons and their properties, Phys. Rev. D 68

2003

Earlier work this paper cites.

T. Damour, A. Gopakumar, and B. R. Iyer, Phasing of gravitational waves from inspiralling eccentric binaries, Phys. Rev. D70

2004

Earlier work this paper cites.

R.-M. Memmesheimer, A. Gopakumar, and G. Schaefer, Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits, Phys. Rev. D 70

2004

Earlier work this paper cites.

M. Ansorg, B. Brügmann, and W. Tichy, A single-domain spectral method for black hole puncture data, Phys. Rev. D70

2004

Earlier work this paper cites.

J. Thornburg, Black hole excision with multiple grid patches, Class.Quant.Grav. 21

2004

Earlier work this paper cites.

O. Dreyer, B. J. Kelly, B. Krishnan, L. S. Finn, D. Garrison, and R. Lopez-Aleman, Black hole spectroscopy: Testing general relativity through gravitational wave observations, Class. Quant. Grav. 21

2004

Earlier work this paper cites.

E. Schnetter, S. H. Hawley, and I. Hawke, Evolutions in 3-D numerical relativity using fixed mesh refinement, Class.Quant.Grav. 21

2004

Earlier work this paper cites.

T. Mora and C. M. Will, A Post-Newtonian diagnostic of quasi-equilibrium binary configurations of compact objects, Phys. Rev. D69

2005

Earlier work this paper cites.

C. Konigsdorffer and A. Gopakumar, Phasing of gravitational waves from inspiralling eccentric binaries at the third-and-a-half post-Newtonian order, Phys. Rev. D 73

2006

Earlier work this paper cites.

M. Campanelli, C. O. Lousto, P. Marronetti, and Y. Zlochower, Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision, Phys. Rev. Lett. 96

2006

Earlier work this paper cites.

J. G. Baker, J. Centrella, D.-I. Choi, M. Koppitz, and J. van Meter, Gravitational wave extraction from an inspiraling configuration of merging black holes, Phys. Rev. Lett. 96

2006

Earlier work this paper cites.

E. Schnetter, B. Krishnan, and F. Beyer, Introduction to dynamical horizons in numerical relativity, Phys. Rev. D 74

2006

Cited alongside, same era.

J. D. Hunter, Matplotlib: A 2d graphics environment, Computing In Science & Engineering 9

2007

Cited alongside, same era.

C. Munna, Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit nonspinning extreme-mass-ratio inspirals to the 19th order, Phys. Rev. D 102

Original

2008

Cited alongside, same era.

P. Marronetti, W. Tichy, B. Brügmann, J. Gonzalez, and U. Sperhake, High-spin binary black hole mergers, Phys.Rev. D77

Original

2008

Cited alongside, same era.

M. Ruiz, R. Takahashi, M. Alcubierre, and D. Nunez, Multipole expansions for energy and momenta carried by gravitational waves, Gen. Rel. Grav. 40

Original

J. Samsing, Eccentric Black Hole Mergers Forming in Globular Clusters, Phys. Rev. D97

Original

2018

Later among the works it cites.

D. Gerosa, E. Berti, R. O’Shaughnessy, K. Belczynski, M. Kesden, D. Wysocki, and W. Gladysz, Spin orientations of merging black holes formed from the evolution of stellar binaries, Phys. Rev. D 98

Original

2018

Later among the works it cites.

M. E. Lower, E. Thrane, P. D. Lasky, and R. Smith, Measuring eccentricity in binary black hole inspirals with gravitational waves, Phys. Rev. D 98

Original

2018

Later among the works it cites.

A. Klein, Y. Boetzel, A. Gopakumar, P. Jetzer, and L. de Vittori, Fourier domain gravitational waveforms for precessing eccentric binaries, Phys. Rev. D98

Original

2018

Later among the works it cites.