The Shape of Eccentricity: Rapid Classification of Eccentric Binaries with the Wavelet Scattering Transform
gr-qc, astro-ph.HE
Submitted: 2026-02-27
Updated: 2026-08-26
Terminology
Sources
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-4.0: Population Properties of Merging Compact Binaries
- Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
- Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars
- A subpopulation of low-mass, spinning black holes: signatures of dynamical assembly
- Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
- Orbital eccentricity in a neutron star - black hole merger
- Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession
- Biased parameter inference of eccentric, spin-precessing binary black holes
- Misinterpreting Spin Precession as Orbital Eccentricity in Gravitational-Wave Signals
- Astrophysical Implications of Eccentricity in Gravitational Waves from Neutron Star-Black Hole Binaries
- Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
- SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
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