Articles Citing

GW200208_222617 as an eccentric black-hole binary merger: Properties and astrophysical implications

Isobel Romero-Shaw ^1,2,3,*, Jakob Stegmann ⁴, Hiromichi Tagawa⁵, Davide Gerosa ^6,7, Johan Samsing⁸, Nihar Gupte ^9,10, and Stephen R. Green ¹¹

¹Department of Applied Mathematics and Theoretical Physics, Cambridge CB3 0WA, United Kingdom
²Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
³H. H. Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol BS8 1TL, United Kingdom
⁴Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany
⁵Shanghai Astronomical Observatory, Shanghai 200030, People’s Republic of China
⁶Dipartimento di Fisica “G. Occhialini,” Università degli Studi di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
⁷INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
⁸Niels Bohr International Academy, The Niels Bohr Institute, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
⁹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
¹⁰Department of Physics, University of Maryland, College Park, Maryland 20742, USA
¹¹School of Mathematical Sciences, University of Nottingham, University Park, Nottingham NG7 2RD, United Kingdom

^*Contact author: isobel.romeroshaw@gmail.com

Parameter estimation with targeted eccentric numerical-relativity simulations for GW200208_22 and GW190620

Patricia McMillin, Katelyn J. Wagner, Giuseppe Ficarra, Carlos O. Lousto, and Richard O’Shaughnessy

Phys. Rev. D 114 024083 (2026)

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects

Gonzalo Morras, Geraint Pratten, Patricia Schmidt, and Alessandra Buonanno

Phys. Rev. D 114 044032 (2026)

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis

Alberto Álvaro-Díaz and Gonzalo Morras

Phys. Rev. D 114 044033 (2026)

Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity

Soumen Roy and Justin Janquart

Phys. Rev. D 114 044075 (2026)

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions

Tousif Islam, Adhrit Ravichandran, Peter James Nee, Scott E. Field, Vijay Varma, Harald P. Pfeiffer, Andrea Ceja, Noora Ghadiri, Lawrence E. Kidder, Prayush Kumar, Marlo Morales, Abhishek Ravishankar, Antoni Ramos-Buades, Katie Rink, Hannes R. Rüter, Mark A. Scheel, Md Arif Shaikh, and Daniel Tellez

Phys. Rev. D 114 044078 (2026)

Misinterpreting spin precession as orbital eccentricity in gravitational-wave signals

Snehal Tibrewal, Aaron Zimmerman, Jacob Lange, and Deirdre Shoemaker

Phys. Rev. D 114 064046 (2026)

Systematic biases in gravitational-wave parameter estimation from neglecting orbital eccentricity in space-based detectors

Jin-Zhao Yang, Jia-Hao Zhong, and Tao Yang

Phys. Rev. D 114 064047 (2026)

Analytical solution of spinning, eccentric binary black hole dynamics at the second post-Newtonian order

Tom Colin, Sashwat Tanay, and Laura Bernard

Phys. Rev. D 114 064051 (2026)

Shape of eccentricity: Rapid classification of eccentric binaries with the wavelet scattering transform

Priscilla Canizares, Seppe J. Staelens, and Isobel Romero-Shaw

Phys. Rev. D 114 083010 (2026)

Revisiting the coprecessing frame in the presence of orbital eccentricity

Lucy M. Thomas, Katerina Chatziioannou, Sam Johar, Taylor Knapp, and Michael Boyle

Phys. Rev. D 114 084090 (2026)

Fast frequency-domain phenomenological modeling of eccentric aligned-spin binary black holes

Antoni Ramos-Buades, Quentin Henry, and Maria Haney

Phys. Rev. D 113 083044 (2026)

Spin-precession effects in the phasing formula of eccentric compact binary inspirals up to the second post-Newtonian order

Soham Bhattacharyya and Omkar Sridhar

Phys. Rev. D 113 084022 (2026)

Biased parameter inference of eccentric, spin-precessing binary black holes

Divyajyoti, Isobel M. Romero-Shaw, Vaishak Prasad, Kaushik Paul, Chandra Kant Mishra, Prayush Kumar, Akash Maurya, Michael Boyle, Lawrence E. Kidder, Harald P. Pfeiffer, and Mark A. Scheel

Phys. Rev. D 113 103022 (2026)

Orbital eccentricity can make neutron star g -mode resonances observable with current gravitational-wave detectors

János Takátsy, Lorenz Zwick, Pankaj Saini, and Johan Samsing

Phys. Rev. D 113 103047 (2026)

Population properties of binary black holes with eccentricity

M. Zeeshan, R. O’Shaughnessy, and N. Malagon

Phys. Rev. D 113 123025 (2026)

Can eccentric binary black hole signals mimic gravitational-wave microlensing?

Anuj Mishra and Apratim Ganguly

Phys. Rev. D 113 123036 (2026)

Test for eccentric binaries based on the spin-induced quadrupole moment

N. V. Krishnendu

Phys. Rev. D 113 124008 (2026)

Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries

Nicholas Loutrel, Ava Bailey, and Davide Gerosa

Class. Quantum Grav. 43 075010 (2026)

GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients

A. G. Abac et al.

ApJL 1004 L21 (2026)

Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples

Jakob Stegmann, Fabio Antonini, Aleksandra Olejak, Sylvia Biscoveanu, Vivien Raymond, Stefano Rinaldi, and Elizabeth Flanagan

ApJL 1000 L59 (2026)

Gravitational Wave Phase Shifts of Black Hole Mergers in AGN Disks

Hiromichi Tagawa, Connar Rowan, János Takátsy, Lorenz Zwick, Kai Hendriks, Wen-Biao Han, and Johan Samsing

ApJ 998 244 (2026)

Eccentricity Constraints Disfavor Single–Single Capture in Nuclear Star Clusters as the Origin of all LIGO–Virgo–KAGRA Binary Black Holes

Nihar Gupte, M. Coleman Miller, Rhiannon Udall, Sophie Bini, Alexandre Toubiana, Alessandra Buonanno, Jonathan Gair, Aldo Gamboa, Lorenzo Pompili, Antoni Ramos-Buades, Maximilian Dax, Stephen R. Green, Annalena Kofler, Jakob Macke, and Bernhard Schölkopf

ApJ 1009 90 (2026)

Properties of Black Hole Mergers in Disks of Active Galactic Nuclei

Hiromichi Tagawa, Zoltán Haiman, and Bence Kocsis

ApJ 1007 67 (2026)

Electromagnetic Flares from Compact-object Mergers in Active Galactic Nucleus Disks: Signatures and Predictions

Hiromichi Tagawa, Zoltán Haiman, Shigeo S. Kimura, Hassen M. Yesuf, and Hengxiao Guo

ApJ 1006 121 (2026)

Inferring Host Environment Properties and Gravitational-wave Decay Time from the Eccentricity Measurement of Dynamically Captured Binaries

A. Vincent Paul, Parthapratim Mahapatra, Marc Favata, and K. G. Arun

ApJ 1006 191 (2026)

Select page:

Physical Review D

Filter

Articles Citing

GW200208_222617 as an eccentric black-hole binary merger: Properties and astrophysical implications

Parameter estimation with targeted eccentric numerical-relativity simulations for GW200208_22 and GW190620

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis

Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions

Misinterpreting spin precession as orbital eccentricity in gravitational-wave signals

Systematic biases in gravitational-wave parameter estimation from neglecting orbital eccentricity in space-based detectors

Analytical solution of spinning, eccentric binary black hole dynamics at the second post-Newtonian order

Shape of eccentricity: Rapid classification of eccentric binaries with the wavelet scattering transform

Revisiting the coprecessing frame in the presence of orbital eccentricity

Fast frequency-domain phenomenological modeling of eccentric aligned-spin binary black holes

Spin-precession effects in the phasing formula of eccentric compact binary inspirals up to the second post-Newtonian order

Biased parameter inference of eccentric, spin-precessing binary black holes

Orbital eccentricity can make neutron star g -mode resonances observable with current gravitational-wave detectors

Population properties of binary black holes with eccentricity

Can eccentric binary black hole signals mimic gravitational-wave microlensing?

Test for eccentric binaries based on the spin-induced quadrupole moment

Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries

GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients

Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples

Gravitational Wave Phase Shifts of Black Hole Mergers in AGN Disks

Eccentricity Constraints Disfavor Single–Single Capture in Nuclear Star Clusters as the Origin of all LIGO–Virgo–KAGRA Binary Black Holes

Properties of Black Hole Mergers in Disks of Active Galactic Nuclei

Electromagnetic Flares from Compact-object Mergers in Active Galactic Nucleus Disks: Signatures and Predictions

Inferring Host Environment Properties and Gravitational-wave Decay Time from the Eccentricity Measurement of Dynamically Captured Binaries

Filter

Filter

Article Lookup

Enter a citation