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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

Eccentric binary black holes: A new framework for numerical relativity waveform surrogates

From the confluent Heun equation to a new factorized and resummed gravitational waveform for circularized, nonspinning, compact binaries

Autoencoder model for fast generation of effective one-body gravitational waveform approximations

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

Theory-agnostic tests of general relativity with a new parametrized model for gravitational waves from eccentric, precessing binary black holes

Rapid inference of gravitational-wave signals in the time domain using a heterodyned likelihood

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

Testing general relativity with amplitudes of subdominant gravitational-wave modes

Modeling the merger-ringdown of an eccentric test-mass inspiral into a Kerr black hole using the effective-one-body framework

Large-eccentricity asymptotics and a fast analytic approximation for Fourier modes of post-Newtonian eccentric waveforms

Ringdown modeling for effective-one-body waveforms in the test-mass limit for eccentric equatorial orbits around a Kerr black hole

Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries

Adiabatic tides in compact binaries on quasielliptic orbits: Dynamics at the second-and-a-half relative post-Newtonian order

Adiabatic tides in compact binaries on quasielliptic orbits: Radiation at the second-and-a-half relative post-Newtonian order

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

Efficient eccentric effective-one-body dynamics via near-identity averaging transformations

High-post-Newtonian-order dynamics induced by tail-of-tail interactions: The nongeodesic terms

Identifiability of g mode resonances in eccentric binary neutron stars with multidetector observations

Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: Parameter estimation and waveform systematics with seobnrv6ehm

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM

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

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