Efficient gravitational-wave model for fully-precessing and moderately eccentric, compact binary inspirals
Author:
Affiliation:
1. University of Illinois at Urbana-Champaign
2. University of Birmingham
Funder
National Aeronautics and Space Administration
National Science Foundation
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.110.044044/fulltext
Reference65 articles.
1. GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run
2. Bayesian inference of binary black holes with inspiral-merger-ringdown waveforms using two eccentric parameters
3. Signs of Eccentricity in Two Gravitational-wave Signals May Indicate a Subpopulation of Dynamically Assembled Binary Black Holes
4. Four Eccentric Mergers Increase the Evidence that LIGO–Virgo–KAGRA’s Binary Black Holes Form Dynamically
5. Measuring eccentricity in binary black hole inspirals with gravitational waves
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