Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition

Abstract

Binary black holes (BBHs) exhibiting spin-induced orbital precession offer unique insight into compact-binary formation channels, cosmology, and tests of general relativity. We conduct a dedicated search for precessing BBHs with unequal masses in Advanced LIGO's third observing run (O3) using the harmonic decomposition method of precessing waveforms. We introduce a novel scheme to reduce the number of filters in a harmonic search. With our new approach, our template bank requires $5\times$ fewer filters compared to another proposed precessing search in the same region. We do not find any new significant events. Our new search method achieves up to $\sim 28\%$ improvement in sensitivity and up to $5\times$ lower computational costs compared to existing precessing search pipelines. Our method enables scalable, sensitive searches for precessing BBHs in future gravitational-wave observing runs.

18 pages, 11 figures. Data release at https://github.com/rahuldhurkunde/O3-precessing-BBH-search. v2 is PRD published version

References in corpus (48)

• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Advanced LIGO
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• A simple model of complete precessing black-hole-binary gravitational waveforms
• The PyCBC search for gravitational waves from compact binary coalescence
• FINDCHIRP: an algorithm for detection of gravitational waves from inspiraling compact binaries
• Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO
• Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
• IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
• Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
• Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit
• Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
• 4-OGC: Catalog of gravitational waves from compact-binary mergers
• Spin orientations of merging black holes formed from the evolution of stellar binaries
• Spin-Orbit Misalignment in Close Binaries with Two Compact Objects
• Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
• Detecting binary compact-object mergers with gravitational waves: Understanding and Improving the sensitivity of the PyCBC search
• New binary black hole mergers in the LIGO--Virgo O3a data
• A stochastic template placement algorithm for gravitational wave data analysis
• Searching for Gravitational Waves from Compact Binaries with Precessing Spins
• The Formation and Gravitational-Wave Detection of Massive Stellar Black-Hole Binaries
• General-relativistic precession in a black-hole binary
• Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
• A physical template family for gravitational waves from precessing binaries of spinning compact objects: Application to single-spin binaries
• Distinguishing short duration noise transients in LIGO data to improve the PyCBC search for gravitational waves from high mass binary black hole mergers
• Detectability of gravitational waves from binary black holes: Impact of precession and higher modes
• A quasi-physical family of gravity-wave templates for precessing binaries of spinning compact objects: Application to double-spin precessing binaries
• Two-harmonic approximation for gravitational waveforms from precessing binaries
• Building a stochastic template bank for detecting massive black hole binaries
• Degeneracies in Sky Localisation Determination from a Spinning Coalescing Binary through Gravitational Wave Observations: a Markov-Chain Monte-Carlo Analysis for two Detectors
• Measuring precession in asymmetric compact binaries
• Template banks to search for compact binaries with spinning components in gravitational wave data
• A single-spin precessing gravitational wave in closed form
• Identifying when Precession can be Measured in Gravitational Waveforms
• Detecting gravitational waves from precessing binaries of spinning compact objects. II. Search implementation for low-mass binaries
• Dynamic Normalization for Compact Binary Coalescence Searches in Non-Stationary Noise
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Searching for Gravitational Waves from the Inspiral of Precessing Binary Systems: Problems with Current Waveforms
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Fourth LIGO-Virgo-KAGRA Observing Run
• Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Sensitivity of spin-aligned searches for neutron star-black hole systems using future detectors
• Precessing Binary Black Holes as Better Dark Sirens
• Constraining the neutron star-black hole merger rate