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Harald P. Pfeiffer ⁷ and Mark A. Scheel ⁸

¹Gravity Exploration Institute, School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
²Department of Physics, Indian Institute of Technology Madras, Chennai 600036, India
³Centre for Strings, Gravitation and Cosmology, Department of Physics, Indian Institute of Technology Madras, Chennai 600036, India
⁴Institute for Gravitation and the Cosmos, Department of Physics, Penn State University, University Park, Pennsylvania 16802, USA
⁵International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560089, India
⁶Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, New York 14853, USA
⁷Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, 14476 Potsdam, Germany
⁸Theoretical Astrophysics 350-17, California Institute of Technology, Pasadena, California 91125, USA

^*Contact author: divyajyoti.physics@gmail.com

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Articles Citing

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

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

Testing general relativity with amplitudes of subdominant gravitational-wave modes

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

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

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

Isolated or dynamical? Tracing black hole binary formation through the population of gravitational-wave sources

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

Eccentricity in disguise? Insights from GW231123 and numerically simulated binary black hole merger signals

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