Searching for asymmetric and heavily precessing Binary Black Holes in the gravitational wave data from the LIGO and Virgo third Observing Run

TL;DR

This paper presents a targeted search for asymmetric, heavily precessing binary black hole mergers in LIGO and Virgo data, improving sensitivity over standard methods and constraining the rate of such systems.

Contribution

The study introduces a specialized matched filtering search using the GstLAL pipeline tailored for precessing binaries, enhancing detection capabilities for these complex systems.

Findings

Detected 30 known gravitational wave events

Placed an upper limit on the merger rate of precessing binaries

No new significant precessing binary candidates found

Abstract

Leveraging the features of the GstLAL pipeline, we present the results of a matched filtering search for asymmetric binary black hole systems with heavily misaligned spins in LIGO and Virgo data taken during the third observing run. Our target systems show strong imprints of precession whereas current searches have non-optimal sensitivity in detecting them. After measuring the sensitivity improvement brought by our search over standard spin-aligned searches, we report the detection of 30 gravitational wave events already discovered in the latest version of the Gravitational Wave Transient Catalog. However, we do not find any additional significant gravitational wave candidates. Our results allow us to place an upper limit of $R_{90\%} = 0.28^{+0.33}_{-0.04}\;\; \mathrm{Gpc^{-3}yr^{-1}}$ on the merger rate of a hypothetical subpopulation of asymmetric, heavily precessing signals, not identified by other searches. Since our upper limit is consistent with the latest rate estimates from the LIGO-Virgo-KAGRA collaboration, our findings rule out the existence of a yet-to-be-discovered population of precessing binaries.