Search for gravitational waves from eccentric binary black holes with an effective-one-body template
Yi-Fan Wang, Alexander H. Nitz

TL;DR
This study conducts the first matched-filtering search for gravitational waves from eccentric binary black holes using an effective-one-body waveform model, identifying known events and setting new constraints on their event rates.
Contribution
It introduces a novel search method for eccentric BBHs with an effective-one-body model and provides the first constraints on their astrophysical event rates.
Findings
Identified 28 BBH events consistent with previous catalogs.
Reported additional candidates with moderate false alarm rates.
Set new upper limits on eccentric BBH event rates, improving sensitivity.
Abstract
As gravitational wave astronomy has entered an era of routine detections, it becomes increasingly important to precisely measure the physical parameters of individual events and infer population properties. Eccentricity is a key observable, suggesting that binaries form in a dense stellar environment through dynamical encounters. This work performs the first matched-filtering search for gravitational waves from eccentric binary black holes (BBHs) covering the mass range and eccentricity at 20 Hz up to 0.5 with a newly developed effective-one-body waveform model. Throughout the third observation run of LIGO, Virgo, and KAGRA, we identify 28 BBH events with a false alarm rate below once per 100 yr; all of which were previously reported in the GWTC-3 and 4-OGC catalogs. Additional candidates with false alarm rates between once per 1 and 100 yr are also reported. We…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
