Black hole - black hole total merger mass and the origin of LIGO/Virgo sources

Abstract

The LIGO-Virgo-KAGRA (LVK) Collaboration has reported nearly 100 BH-BH mergers. The LVK provides estimates of rates, masses, effective spins, and redshifts for these mergers. Yet, the formation channel(s) of the mergers remains uncertain. One way to search for a formation site is to contrast properties of detected BH-BH mergers with different models of BH-BH merger formation. Our study is designed to investigate the usefulness of the total BH-BH merger mass and its evolution with redshift in establishing the origin of gravitational-wave sources. We find that the average intrinsic BH-BH total merger mass shows exceptionally different behavior for the models that we adopt for our analysis. In the local universe (z=0) the average merger mass changes from Mtot,int=25Msun for CE binary evolution and open clusters formation channels, to Mtot,int=30Msun for the stable-RLOF binary channel, to Mtot,int=45Msun for the globular cluster channel. These differences are even more pronounced at larger redshifts. However, these differences are diminished when considering LVK O3 detector sensitivity. Comparison with LVK O3 data shows that none of our adopted models can match the data despite large errors on BH-BH masses and redshifts. We emphasize that our conclusions are derived from a small set of 6 models that are subject to numerous known uncertainties. We also note that BH-BH mergers may originate from a mix of several channels and that other (than those adopted here) BH-BH formation channels may exist.

arXiv commentApJ: accepted. Revised and updated version

References in corpus (117)

• On the variation of the Initial Mass Function
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• Binary interaction dominates the evolution of massive stars
• Evolution of binary stars and the effect of tides on binary populations
• 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
• A statistical study of 233 pulsar proper motions
• Mind your Ps and Qs: the Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars
• Young massive star clusters
• The propagation of uncertainties in stellar population synthesis modeling III: model calibration, comparison, and evaluation
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
• The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
• Compact Object Modeling with the StarTrack Population Synthesis Code
• Black Hole Formation in Failing Core-Collapse Supernovae
• Ultraluminous X-Ray Sources in External Galaxies
• Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
• Black hole mergers in the universe
• On The Maximum Mass of Stellar Black Holes
• A new route towards merging massive black holes
• Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
• The Effects of Binary Evolution on the Dynamics of Core Collapse and Neutron-Star Kicks
• Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
• The VLT-FLAMES Tarantula Survey VIII. Multiplicity properties of the O-type star population
• On the metallicity dependence of Wolf-Rayet winds
• The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• The Neutron Star and Black Hole Initial Mass Function
• The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes
• The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks
• MOCCA-SURVEY Database I: Coalescing Binary Black Holes Originating From Globular Clusters
• On the formation and evolution of black-hole binaries
• Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties
• Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries
• Binary black hole mergers from field triples: properties, rates and the impact of stellar evolution
• The effect of metallicity on the detection prospects for gravitational waves
• Most Black Holes are Born Very Slowly Rotating
• One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
• The effect of the metallicity-specific star formation history on double compact object mergers
• Massive black hole binaries from runaway collisions: the impact of metallicity
• Merging black hole binaries with the SEVN code
• Stellar-mass black holes in star clusters: implications for gravitational wave radiation
• Missing Black Holes Unveil The Supernova Explosion Mechanism
• Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries
• Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers
• Galactic distribution of merging neutron stars and black holes - prospects for short GRB progenitors and LIGO/VIRGO
• Accelerating NBODY6 with Graphics Processing Units
• Dynamical Formation of the GW150914 Binary Black Hole
• Rates of Compact Object Coalescences
• The spin of the second-born black hole in coalescing binary black holes
• On the rarity of double black hole binaries: consequences for gravitational-wave detection
• Constraints from gravitational wave detections of binary black hole mergers on the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ rate
• Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
• Implementing Few-Body Algorithmic Regularization with Post-Newtonian Terms
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation
• Stability of mass transfer from massive giants: double black-hole binary formation and ultra-luminous X-ray sources
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• Monte-Carlo Simulations of Globular Cluster Evolution - I. Method and Test Calculations
• Low metallicity natal environments and black hole masses in Ultraluminous X-ray Sources
• The impact of pair-instability mass loss on the binary black hole mass distribution
• The formation and hierarchical assembly of globular cluster populations
• Stellar Collisions and the Interior Structure of Blue Stragglers
• Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties
• 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
• It has to be cool: on supergiant progenitors of binary black hole mergers from common-envelope evolution
• The impact of mass-transfer physics on the observable properties of field binary black hole populations
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation II
• The redshift evolution of the binary black hole merger rate: a weighty matter
• Populating the upper black hole mass gap through stellar collisions in young star clusters
• Binary black holes in young star clusters: the impact of metallicity
• BSE versus StarTrack: implementations of new wind, remnant-formation, and natal-kick schemes in NBODY7 and their astrophysical consequences
• Exploring the Lower Mass Gap and Unequal Mass Regime in Compact Binary Evolution
• Redshift Evolution of the Black Hole Merger Rate from Globular Clusters
• Distance measures in gravitational-wave astrophysics and cosmology
• Distribution of Effective Spins and Masses of Binary Black Holes from the LIGO and Virgo O1-O3a Observing Runs
• Binary Black Holes in Dense Star Clusters: Exploring the Theoretical Uncertainties
• Common Envelope Wind Tunnel: Coefficients of Drag and Accretion in a Simplified Context for Studying Flows Around Objects Embedded Within Stellar Envelopes
• MOCCA-SURVEY Database I. Unravelling black hole subsystems in globular clusters
• Stellar-mass black holes in young massive and open stellar clusters IV: updated stellar-evolutionary and black hole spin models and comparisons with the LIGO-Virgo O1/O2 merger-event data
• Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates
• Pulsational Pair-instability Supernovae. I. Pre-collapse Evolution and Pulsational Mass Ejection
• The most ordinary formation of the most unusual double black hole merger
• Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
• Mergers and ejections of black holes in globular clusters
• Is GW190521 the merger of black holes from the first stellar generations?
• A Parallel Monte Carlo Code for Simulating Collisional N-body Systems
• Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in nuclear star clusters
• The Emergence of Structure in the Binary Black Hole Mass Distribution
• Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2
• Equation of state effects in the core collapse of a $20$-$M_{\odot }$ star
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Metallicity of stars formed throughout the cosmic history based on the observational properties of star forming galaxies
• The impact of common envelope development criteria on the formation of LIGO/Virgo sources
• When are LIGO/Virgo's Big Black-Hole Mergers?
• Formation of Binary Black Holes Similar to GW190521 with a Total Mass of $\sim 150M_{\odot }$ from Population III Binary Star Evolution
• The implications of high BH spins on the origin of BH-BH mergers
• Exploring Features in the Binary Black Hole Population
• The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
• Stellar Black Hole Binary Mergers in Open Clusters
• Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
• Ain't No Mountain High Enough: Semi-Parametric Modeling of LIGO-Virgos Binary Black Hole Mass Distribution
• Mixing in massive stellar mergers
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation III: dissecting black hole dynamics
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• On the origin of the mass-metallicity gradient relation in the local Universe
• Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems
• Dynamics of binary black holes in low-mass young star clusters
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• Demographics of neutron stars in young massive and open clusters
• Convective overshoot mixing in stellar interior models
• The connection between merging double compact objects and the Ultraluminous X-ray Sources
• The MEGaN project I. Missing formation of massive nuclear clusters and tidal disruption events by star clusters - massive black hole interactions
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• LISA sources from young massive and open stellar clusters
• Dynamical double black holes and their host cluster properties

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• The Science of the Einstein Telescope
• Do unequal-mass binary black hole systems have larger ${\chi }_{\text{eff}}$? Probing correlations with copulas in gravitational-wave astronomy
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Evidence for a correlation between binary black hole mass ratio and black-hole spins
• Isolated and dynamical black hole mergers with \texttt{B-POP}: the role of star formation and dynamics, star cluster evolution, natal kicks, mass and spins, and hierarchical mergers
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• The role of stellar expansion on the formation of gravitational wave sources
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• Spin Doctors: How to diagnose a hierarchical merger origin
• Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Gravitational wave mergers of accreting binary black holes in AGN discs
• What's in a binary black hole's mass parameter?
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• Joint estimation of the cosmological model and the mass and redshift distributions of the binary black hole population with the Einstein Telescope