Defining eccentricity for gravitational wave astronomy
Md Arif Shaikh(University of Utah), Maarten van de Meent(Max Planck Institute for Gravitational Physics), Harald Pfeiffer(Max Planck Institute for Gravitational Physics), A. Ramos-Buades(Max Planck Institute for Gravitational Physics), Vijay Varma(University of Massachusetts Dartmouth)
Cited by 59
Related Papers
Computationally efficient models for the dominant and subdominant harmonic modes of precessing binary black holes
|Physical review. D/Physical review. D.|2021|543
Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries
|Physical review. D/Physical review. D.|2020|308
Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes
|Physical review. D/Physical review. D.|2020|279
Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
|Physical review. D/Physical review. D.|2023|140
Laying the foundation of the effective-one-body waveform models SEOBNRv5: Improved accuracy and efficiency for spinning nonprecessing binary black holes
|Physical review. D/Physical review. D.|2023|134