Articles Citing

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model seobnrv5ehm

Aldo Gamboa ^1,*, Alessandra Buonanno ^1,2, Raffi Enficiaud ¹, Mohammed Khalil ³, Antoni Ramos-Buades ⁴, Lorenzo Pompili ¹, Héctor Estellés ¹, Michael Boyle ⁵, Lawrence E. Kidder ⁵ et al.

Harald P. Pfeiffer ¹, Hannes R. Rüter ^1,6, and Mark A. Scheel ⁷

¹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
²Department of Physics, University of Maryland, College Park, Maryland 20742, USA
³Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2L 2Y5, Canada
⁴Nikhef, Science Park 105, 1098 XG, Amsterdam, The Netherlands
⁵Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, New York 14853, USA
⁶CENTRA, Departamento de Física, Instituto Superior Técnico—IST, Universidade de Lisboa—UL, Avenida Rovisco Pais 1, 1049-001 Lisboa, Portugal
⁷Theoretical Astrophysics 350-17, California Institute of Technology, Pasadena, California 91125, USA

^*Contact author: aldo.gamboa@aei.mpg.de

Black Hole Spectroscopy and Tests of General Relativity with GW250114

A. G. Abac et al.

Phys. Rev. Lett. 136 041403 (2026)

Scalar Fields around Black Hole Binaries in LIGO-Virgo-KAGRA

Soumen Roy, Rodrigo Vicente, Josu C. Aurrekoetxea, Katy Clough, and Pedro G. Ferreira

Phys. Rev. Lett. 136 191402 (2026)

Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits

Maria de Lluc Planas, Antoni Ramos-Buades, Cecilio García-Quirós, Héctor Estellés, Sascha Husa, and Maria Haney

Phys. Rev. D 113 024006 (2026)

GW200105: A detailed study of eccentricity in the neutron star-black hole binary

Aasim Jan, Bing-Jyun Tsao, Richard O’Shaughnessy, Deirdre Shoemaker, and Pablo Laguna

Phys. Rev. D 113 024018 (2026)

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

Héctor Estellés, Alessandra Buonanno, Raffi Enficiaud, Cheng Foo, and Lorenzo Pompili

Phys. Rev. D 113 044049 (2026)

Binary black hole merger in the extreme mass ratio limit: A multipolar analysis of the inclined orbit case

Luca Nagni, Alessandro Nagar, Rossella Gamba, Simone Albanesi, and Sebastiano Bernuzzi

Phys. Rev. D 113 044052 (2026)

Hybrid waveform model for asymmetric spinning binaries: Self-force meets post-Newtonian theory

Loïc Honet, Adam Pound, and Geoffrey Compère

Phys. Rev. D 113 064035 (2026)

Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession

Yumeng Xu, Jorge Valencia, Héctor Estellés Estrella, Antoni Ramos-Buades, Sascha Husa, Maria Rosselló-Sastre, Joan Llobera Querol, Felip A. Ramis Vidal, Maria de Lluc Planas Llompart, Marta Colleoni, Eleanor Hamilton, Arnau Montava Agudo, Jesús Yébana Carrilero, and Anna Heffernan

Phys. Rev. D 113 083001 (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)

Exploring the gauge flexibility of the linear-in-spin effective-one-body Hamiltonian at the 5.5 post-Newtonian order

Andrea Placidi, Luca Sebastiani, and Gianluca Grignani

Phys. Rev. D 113 084009 (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)

Improved gravitational wave model linking precessing inspirals and numerical-relativity-calibrated merger-ringdown

Eleanor Hamilton, Marta Colleoni, Jonathan E. Thompson, Charlie Hoy, Anna Heffernan, Meryl Kinnear, Jorge Valencia, Felip A. Ramis Vidal, Cecilio García-Quirós, Shrobana Ghosh, Lionel London, Mark Hannam, and Sascha Husa

Phys. Rev. D 113 084055 (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)

Comprehensive look into the accuracy of spectral Einstein code binary black hole waveforms

Taylor Knapp, Katerina Chatziioannou, Keefe Mitman, Mark A. Scheel, Michael Boyle, Lawrence E. Kidder, and Harald Pfeiffer

Phys. Rev. D 113 124001 (2026)

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

Nami Nishimura, Alessandra Buonanno, Guglielmo Faggioli, Maarten van de Meent, and Gaurav Khanna

Phys. Rev. D 113 124034 (2026)

Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests

Simone Mezzasoma, Carl-Johan Haster, and Nicolás Yunes

Phys. Rev. D 113 124043 (2026)

Plunge-merger-ringdown tests of general relativity with GW250114

Leonardo Grimaldi, Elisa Maggio, Lorenzo Pompili, and Alessandra Buonanno

Phys. Rev. D 113 L061506 (2026)

Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses

C Hoy

Monthly Notices of the Royal Astronomical Society 549 stag898 (2026)

Astrophysical implications of eccentricity in gravitational waves from neutron star-black hole binaries

Isobel Romero-Shaw, Jakob Stegmann, Gonzalo Morras, Andris Dorozsmai, and Michael Zevin

Monthly Notices of the Royal Astronomical Society 547 stag323 (2026)

The Science of the Einstein Telescope

Adrian Abac et al.

J. Cosmol. Astropart. Phys. 2026 081 (2026)

Orbital Eccentricity in a Neutron Star–Black Hole Merger

Gonzalo Morras, Geraint Pratten, and Patricia Schmidt

ApJL 1000 L2 (2026)

GW250114: Testing Hawking’s Area Law and the Kerr Nature of Black Holes

A. G. Abac et al.

Phys. Rev. Lett. 135 111403 (2025)

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model seobnrv5ehm

Aldo Gamboa, Mohammed Khalil, and Alessandra Buonanno

Phys. Rev. D 112 044037 (2025)

Select page:

Physical Review D

Filter

Articles Citing

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model seobnrv5ehm

Black Hole Spectroscopy and Tests of General Relativity with GW250114

Scalar Fields around Black Hole Binaries in LIGO-Virgo-KAGRA

Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits

GW200105: A detailed study of eccentricity in the neutron star-black hole binary

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

Binary black hole merger in the extreme mass ratio limit: A multipolar analysis of the inclined orbit case

Hybrid waveform model for asymmetric spinning binaries: Self-force meets post-Newtonian theory

Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession

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

Exploring the gauge flexibility of the linear-in-spin effective-one-body Hamiltonian at the 5.5 post-Newtonian order

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

Improved gravitational wave model linking precessing inspirals and numerical-relativity-calibrated merger-ringdown

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

Comprehensive look into the accuracy of spectral Einstein code binary black hole waveforms

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

Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests

Plunge-merger-ringdown tests of general relativity with GW250114

Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses

Astrophysical implications of eccentricity in gravitational waves from neutron star-black hole binaries

The Science of the Einstein Telescope

Orbital Eccentricity in a Neutron Star–Black Hole Merger

GW250114: Testing Hawking’s Area Law and the Kerr Nature of Black Holes

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model seobnrv5ehm

Filter

Filter

Article Lookup

Enter a citation