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¹Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, 07743, Jena, Germany
²INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy
³Institute for Gravitation and The Cosmos, The Pennsylvania State University, University Park, Pennsylvania 16802, USA
⁴Department of Physics, University of California, Berkeley, CA 94720, USA
⁵Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, Martí i Franquès 1, E-08028 Barcelona, Spain
⁶Institut d’Aplicacions Computacionals i de Codi Comunitari (IAC3)—IEEC, Universitat de les Illes Balears, Carretera Valldemossa km 7.5, E-07122 Palma, Spain
⁷Institut des Hautes Etudes Scientifiques, 91440 Bures-sur-Yvette, France

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Articles Citing

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

Identification and characterization of distorted gravitational waves by lensing using deep learning

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

Covariant and gauge-invariant metric-based gravitational-waves extraction in numerical relativity

Nonlinear stability of rotating hairy black holes

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

High-order effective-one-body tidal interactions and gravitational scattering

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

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

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