Reconstructing the Genealogy of LIGO-Virgo Black Holes

Abstract

We propose a Bayesian inference framework to predict the merger history of LIGO-Virgo binary black holes (BHs), whose binary components may have undergone hierarchical mergers in the past. The framework relies on numerical relativity predictions for the mass, spin, and kick velocity of the remnant BHs. This proposed framework computes the masses, spins, and kicks imparted to the remnant of the parent binaries, given the initial masses and spin magnitudes of the binary constituents. We validate our approach by performing an ``injection study'' based on a constructed sequence of hierarchically formed binaries. Noise is added to the final binary in the sequence, and the parameters of the `parent' and `grandparent' binaries in the merger chain are then reconstructed. This method is then applied to three GWTC-3 events: GW190521, GW200220_061928, and GW190426_190642. These events were selected because at least one of the binary companions lies in the putative pair-instability supernova mass gap, in which stellar processes alone cannot produce BHs. Hierarchical mergers offer a natural explanation for the formation of BHs in the pair-instability mass gap. We use the backward evolution framework to predict the parameters of the parents of the primary companion of these three binaries. For instance, the parent binary of GW190521 has masses $72_{-22}^{+32}{M}_{\odot }$ and $31_{-23}^{+24}{M}_{\odot }$ within the 90% credible interval. Astrophysical environments with escape speeds $\ge 100\mathrm{km}{\mathrm{s}}^{-1}$ are preferred sites to host these events. Our approach can be readily applied to future high-mass gravitational wave events to predict their formation history under the hierarchical merger assumption.

arXiv comment21 pages, 8 figures, 5 tables

References in corpus (104)

• Planck 2015 results. XIII. Cosmological parameters
• On the variation of the Initial Mass Function
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Advanced LIGO
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
• How Massive Single Stars End their Life
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
• Mass-loss predictions for O and B stars as a function of metallicity
• Evolution of Binary Black Hole Spacetimes
• Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Gravitational wave extraction from an inspiraling configuration of merging black holes
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
• Pulsational Pair-Instability Supernovae
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Pulsational pair instability as an explanation for the most luminous supernovae
• Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
• Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• Scientific Objectives of Einstein Telescope
• Large Merger Recoils and Spin Flips From Generic Black-Hole Binaries
• Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue
• Production of Intermediate-Mass Black Holes in Globular Clusters
• Total recoil: the maximum kick from nonspinning black-hole binary inspiral
• Surrogate models for precessing binary black hole simulations with unequal masses
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections
• Consequences of gravitational radiation recoil
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• Supermassive recoil velocities for binary black-hole mergers with antialigned spins
• Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
• Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties
• Binary Mergers and Growth of Black Holes in Dense Star Clusters
• Are merging black holes born from stellar collapse or previous mergers?
• Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
• GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal
• Hierarchical Black Hole Mergers in Active Galactic Nuclei
• Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
• Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections
• Constraints from gravitational wave detections of binary black hole mergers on the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ rate
• How black holes get their kicks: Gravitational radiation recoil revisited
• Predicting the direction of the final spin from the coalescence of two black holes
• Pulsational pair-instability supernovae in very close binaries
• The Pair-Instability Mass Gap for Black Holes
• Gravitational Recoil From Accretion-Aligned Black-Hole Binaries
• Remnant Masses, Spins and Recoils from the Merger of Generic Black-Hole Binaries
• Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and ${}^{12}$C($\alpha$, $\gamma$)${}^{16}$O rate on the pair-instability black hole mass gap
• Remnant mass, spin, and recoil from spin aligned black-hole binaries
• Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties
• Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation II
• Populating the upper black hole mass gap through stellar collisions in young star clusters
• Mass-gap Mergers in Active Galactic Nuclei
• On the mass radiated by coalescing black-hole binaries
• High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants
• Binary black holes in the pair-instability mass gap
• Further insight into gravitational recoil
• Binary black hole mergers: large kicks for generic spin orientations
• Spin Evolution of Stellar-mass Black Hole Binaries in Active Galactic Nuclei
• Black hole genealogy: Identifying hierarchical mergers with gravitational waves
• Hierarchical Black-Hole Mergers in Multiple Systems: Constrain the Formation of GW190412, GW190814 and GW190521-like events
• Gravitational Waves and Intermediate-mass Black Hole Retention in Globular Clusters
• Minding the gap: GW190521 as a straddling binary
• 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
• Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap
• Repeated mergers and ejection of black holes within nuclear star clusters
• Merger rate density of Population III binary black holes below, above, and in the pair-instability mass gap
• Intermediate-mass Black Holes from High Massive-star Binary Fractions in Young Star Clusters
• Is GW190521 the merger of black holes from the first stellar generations?
• PRECESSION: Dynamics of spinning black-hole binaries with python
• Predictions for the hydrogen-free ejecta of pulsational pair-instability supernovae
• A new channel to form IMBHs throughout cosmic time
• The Emergence of Structure in the Binary Black Hole Mass Distribution
• The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae
• Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
• Nonlinear Gravitational Recoil from the Mergers of Precessing Black-Hole Binaries
• Formation of Binary Black Holes Similar to GW190521 with a Total Mass of $\sim 150M_{\odot }$ from Population III Binary Star Evolution
• Formation of GW190521 via gas accretion onto Population III stellar black hole remnants born in high-redshift minihalos
• Coalescing black hole binaries from globular clusters: mass distributions and comparison to gravitational wave data from GWTC-3
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• Resolving the Stellar-Collapse and Hierarchical-Merger origins of the Coalescing Black Holes
• GW190412 as a Third-Generation Black Hole Merger from a Super Star Cluster
• Black holes in the low mass gap: Implications for gravitational wave observations
• Remnant Black Hole Kicks and Implications for Hierarchical Mergers
• Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
• Generation of massive stellar black holes by rapid gas accretion in primordial dense clusters
• Astrophysical implications of GW190412 as a remnant of a previous black-hole merger
• Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function
• Limits on hierarchical black hole mergers from the most negative ${\chi }_{\mathrm{eff}}$ systems
• Correlations in gravitational-wave reconstructions from eccentric binaries: A case study with GW151226 and GW170608
• Black Hole Leftovers: The Remnant Population from Binary Black Hole Mergers
• Looking for the parents of LIGO's black holes
• Growth of stellar mass black holes in dense molecular clouds and GW190521
• Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum
• Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters
• Binary black holes mergers from hierarchical triples in open clusters
• Ancestral Black Holes of Binary Merger GW190521
• Extending black-hole remnant surrogate models to extreme mass ratios
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries

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