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

Gonzalo Morras ^1,2,*, Geraint Pratten ³, Patricia Schmidt ³, and Alessandra Buonanno ^1,4

¹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
²Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, Cantoblanco 28049 Madrid, Spain
³School of Physics and Astronomy and Institute for Gravitational Wave Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom
⁴Department of Physics, University of Maryland, College Park, Maryland 20742, USA

^*Contact author: gonzalo.morras@aei.mpg.de

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Articles Citing

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

Spin-Inversion Degeneracies in Restricted Inspiral Waveforms for LISA

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

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

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

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