Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo

Abstract

Intermediate-mass black holes (IMBHs) span the approximate mass range $100$--$10^5{M}_{\odot }$, between black holes (BHs) formed by stellar collapse and the supermassive BHs at the centers of galaxies. Mergers of IMBH binaries are the most energetic gravitational-wave sources accessible by the terrestrial detector network. Searches of the first two observing runs of Advanced LIGO and Advanced Virgo did not yield any significant IMBH binary signals. In the third observing run (O3), the increased network sensitivity enabled the detection of GW190521, a signal consistent with a binary merger of mass $\sim 150M_{\odot }$ providing direct evidence of IMBH formation. Here we report on a dedicated search of O3 data for further IMBH binary mergers, combining both modelled (matched filter) and model independent search methods. We find some marginal candidates, but none are sufficiently significant to indicate detection of further IMBH mergers. We quantify the sensitivity of the individual search methods and of the combined search using a suite of IMBH binary signals obtained via numerical relativity, including the effects of spins misaligned with the binary orbital axis, and present the resulting upper limits on astrophysical merger rates. Our most stringent limit is for equal mass and aligned spin BH binary of total mass $200M_{\odot }$ and effective aligned spin 0.8 at $0.056Gp{c}^{-3}y{r}^{-1}$ (90 $\%$ confidence), a factor of 3.5 more constraining than previous LIGO-Virgo limits. We also update the estimated rate of mergers similar to GW190521 to $0.08Gp{c}^{-3}y{r}^{-1}$.

Main paper: 12 pages and 2 figures; total 27 pages with appendices and 4 figures

References in corpus (52)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• X-ray Properties of Black-Hole Binaries
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
• An Ultraluminous X-ray Source Powered by An Accreting Neutron Star
• Pulsational Pair-Instability Supernovae
• Pulsational pair instability as an explanation for the most luminous supernovae
• Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Total recoil: the maximum kick from nonspinning black-hole binary inspiral
• An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907
• BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
• Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
• Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
• Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
• Observational evidence for intermediate-mass black holes
• Merging black holes in young star clusters
• The Evolution of Massive Helium Stars Including Mass Loss
• Gemini and Hubble Space Telescope Evidence for an Intermediate Mass Black Hole in omega Centauri
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit
• Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
• The Pair-Instability Mass Gap for Black Holes
• Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
• The BayesWave analysis pipeline in the era of gravitational wave observations
• Testing the no-hair theorem with black hole ringdowns using TIGER
• Characterization of systematic error in Advanced LIGO calibration
• Mass-gap Mergers in Active Galactic Nuclei
• Machine-learning non-stationary noise out of gravitational wave detectors
• Localization of gravitational wave sources with networks of advanced detectors
• GW190521 may be an intermediate mass ratio inspiral
• Polluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries
• Observing IMBH-IMBH Binary Coalescences via Gravitational Radiation
• The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst
• The Loudest Event Statistic: General Formulation, Properties and Applications
• Accelerating parameter inference with graphics processing units
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• A Bayesian approach to the follow-up of candidate gravitational wave signals
• The Formation of a 70 Msun Black Hole at High Metallicity
• Generation of massive stellar black holes by rapid gas accretion in primordial dense clusters
• Challenges testing the no-hair theorem with gravitational waves
• On the radio properties of the intermediate-mass black hole candidate ESO 243-49 HLX-1
• The GstLAL Search Analysis Methods for Compact Binary Mergers in Advanced LIGO's Second and Advanced Virgo's First Observing Runs
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Pulsational pair-instability and the mass gap of Population III Black Holes: Effects of overshooting
• Incorporation of Statistical Data Quality Information into the GstLAL Search Analysis

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• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• 4-OGC: Catalog of gravitational waves from compact-binary mergers
• GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot }$
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• The Science of the Einstein Telescope
• Data quality up to the third observing run of Advanced LIGO: Gravity Spy glitch classifications
• Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
• Unveiling the merger structure of black hole binaries in generic planar orbits
• First gravitational-wave search for intermediate-mass black hole mergers with higher order harmonics
• Eccentricity of Long Inspiraling Compact Binaries Sheds Light on Dark Sirens
• Binary black hole mergers from young massive clusters in the pair-instability supernova mass gap
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data
• New search pipeline for gravitational waves with higher-order modes using mode-by-mode filtering
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Splitting the lentils: Clues to galaxy/black hole coevolution from the discovery of offset relations for non-dusty versus dusty (wet-merger-built) lenticular galaxies in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ diagram
• Exploring field-evolution and dynamical-capture coalescing binary black holes in GWTC-3
• Observational limits on the rate of radiation-driven binary black hole capture events
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• Extragalactic neutrino emission induced by Supermassive and Stellar Mass Black Hole mergers
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Searching for gravitational-wave bursts with space-borne detectors
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• A Unified $p_{\mathrm{astro}}$ for Gravitational Waves: Consistently Combining Information from Multiple Search Pipelines
• Enhancing search pipelines for short gravitational wave transients with Gaussian mixture modelling
• Type Ia supernova constraints on compact object dark matter
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Intermediate-mass-ratio inspirals with general dynamical friction in dark matter minispikes
• Eccentric mergers of binary Proca stars
• The impact of local noise recorded at the ET candidate sites on the signal to noise ratio of CBC gravitational wave signals for the ET triangle configuration
• MOCCA-Survey Database: Extra Galactic Globular Clusters. III. The population of black holes in Milky Way and Andromeda-like galaxies
• Possible Gravitational Microlensing Events in the Optical Lightcurve of Active Galaxy S5 0716+714
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Master functions of Reissner-Nordstrom black hole perturbations and their Darboux transformation
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Scattered light reduction in Sagnac Speed Meters with Tunable Coherence
• Merger rates of intermediate-mass black hole binaries in nuclear star clusters
• Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
• Observing GW190521-like binary black holes and their environment with LISA