The impact of pair-instability mass loss on the binary black hole mass distribution

Abstract

A population of binary black hole mergers has now been observed in gravitational waves by Advanced LIGO and Virgo. The masses of these black holes appear to show evidence for a pile-up between $30$--$45$ $M_{\odot }$ and a cut-off above $\sim 45$ $M_{\odot }$. One possible explanation for such a pile-up and subsequent cut-off are pulsational pair-instability supernovae (PPISNe) and pair-instability supernovae (PISNe) in massive stars. We investigate the plausibility of this explanation in the context of isolated massive binaries. We study a population of massive binaries using the rapid population synthesis software COMPAS, incorporating models for PPISNe and PISNe. Our models predict a maximum black hole mass of $40$ $M_{\odot }$. We expect $\sim 10$\% of all binary black hole mergers at redshift z = 0 will include at least one component that went through a PPISN (with mass $30$--$40$ $M_{\odot }$), constituting $\sim 20$--$50$\% of binary black hole mergers observed during the first two observing runs of Advanced LIGO and Virgo. Empirical models based on fitting the gravitational-wave mass measurements to a combination of a power law and a Gaussian find a fraction too large to be associated with PPISNe in our models. The rates of PPISNe and PISNe track the low metallicity star formation rate, increasing out to redshift $z=2$. These predictions may be tested both with future gravitational-wave observations and with observations of superluminous supernovae.

arXiv comment16 pages, 9 figures, accepted to ApJ, data available at www.compas.science

References in corpus (120)

• Astropy: A Community Python Package for Astronomy
• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
• On the variation of the Initial Mass Function
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• Modules for Experiments in Stellar Astrophysics (MESA)
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Cosmic Star Formation History
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• Binary interaction dominates the evolution of massive stars
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• Evolution of binary stars and the effect of tides on binary populations
• A Survey of Stellar Families: Multiplicity of Solar-Type Stars
• 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
• Characterization of the LIGO detectors during their sixth science run
• Did LIGO detect dark matter?
• Mind your Ps and Qs: the Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars
• Common Envelope Evolution: Where we stand and how we can move forward
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
• Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
• Pulsational Pair-Instability Supernovae
• Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
• Pulsational pair instability as an explanation for the most luminous supernovae
• On The Maximum Mass of Stellar Black Holes
• A new route towards merging massive black holes
• Luminous Supernovae
• Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei
• Hydrogen-poor superluminous stellar explosions
• Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
• Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"
• Pair-Instability Supernovae, Gravity Waves, and Gamma-Ray Transients
• Supernova 2007bi as a pair-instability explosion
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE
• Formation of the first three gravitational-wave observations through isolated binary evolution
• Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
• New binary black hole mergers in the second observing run of Advanced LIGO and Advanced Virgo
• Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
• 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
• Are merging black holes born from stellar collapse or previous mergers?
• Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
• The search for failed supernovae with the Large Binocular Telescope: confirmation of a disappearing star
• On the formation history of Galactic double neutron stars
• Merging black hole binaries with the SEVN code
• Slowly fading super-luminous supernovae that are not pair-instability explosions
• Merging black holes in young star clusters
• BPASS predictions for Binary Black-Hole Mergers
• Distance measures in cosmology
• Are LIGO's Black Holes Made From Smaller Black Holes?
• Does the Black Hole Merger Rate Evolve with Redshift?
• An excess of massive stars in the local 30 Doradus starburst
• Measuring the binary black hole mass spectrum with an astrophysically motivated parameterization
• Dynamical Formation of the GW150914 Binary Black Hole
• The Evolution of Massive Helium Stars Including Mass Loss
• On the rarity of double black hole binaries: consequences for gravitational-wave detection
• Investigating stellar-mass black hole kicks
• Evolution of massive population III stars with rotation and magnetic fields
• Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
• A Highly Spinning and Aligned Binary Black Hole Merger in the Advanced LIGO First Observing Run
• Merging stellar-mass binary black holes
• On the Collapsar Model of Long Gamma-Ray Bursts: Constraints from Cosmic Metallicity Evolution
• Where are LIGO's Big Black Holes?
• On the Binding Energy Parameter $\lambda$ of Common Envelope Evolution
• Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
• Black hole mergers from an evolving population of globular clusters
• Rates of Superluminous Supernovae at z~0.2
• Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
• Effects of Rotation on the Minimum Mass of Primordial Progenitors of Pair Instability Supernovae
• Stability of mass transfer from massive giants: double black-hole binary formation and ultra-luminous X-ray sources
• Super-luminous supernovae at redshifts of 2.05 and 3.90
• The Search for Failed Supernovae with The Large Binocular Telescope: First Candidates
• Massive main sequence stars evolving at the Eddington limit
• Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
• Natal Kicks of Stellar-Mass Black Holes by Asymmetric Mass Ejection in Fallback Supernovae
• Estimates of black-hole natal kick velocities from observations of low-mass X-ray binaries
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• Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star
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• A Systematic Survey of the Effects of Wind Mass Loss Algorithms on the Evolution of Single Massive Stars
• Black hole mergers from quadruples
• A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo
• Accuracy of inference on the physics of binary evolution from gravitational-wave observations
• Constraints on Binary Black Hole Populations from LIGO-Virgo Detections
• A consistent estimate for Gravitational Wave and Electromagnetic transient rates
• Black hole formation and fallback during the supernova explosion of a $40{\mathrm{M}}_{\odot }$ star
• The Black Hole Mass Function from Gravitational Wave Measurements
• The influence of the distribution of cosmic star formation at different metallicities on the properties of merging double compact objects
• The Galactic distribution of X-ray binaries and its implications for compact object formation and natal kicks
• Related progenitor models for long-duration gamma ray bursts and Type Ic superluminous supernovae
• Distinguishing compact binary population synthesis models using gravitational-wave observations of coalescing binary black holes
• Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae
• The Volumetric Rate of Superluminous Supernovae at z~1
• Explaining LIGO's observations via isolated binary evolution with natal kicks
• Dynamical Formation of Low-Mass Merging Black Hole Binaries like GW151226
• The metallicity dependence of envelope inflation in massive stars
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• PS1-14bj: A Hydrogen-Poor Superluminous Supernova With a Long Rise and Slow Decay
• Fast evolving pair-instability supernova models: evolution, explosion, light curves
• Observational properties of low redshift pair instability supernovae
• Stellar Black Hole Binary Mergers in Open Clusters
• Explosion and nucleosynthesis of low redshift pair instability supernovae
• Parameter estimation on compact binary coalescences with abruptly terminating gravitational waveforms
• Pulsations of red supergiant pair-instability supernova progenitors leading to extreme mass loss
• Models for the Unusual Supernova iPTF14hls
• Can pair-instability supernova models match the observations of superluminous supernovae?
• First release of high-redshift superluminous supernovae from the Subaru HIgh-Z sUpernova CAmpaign (SHIZUCA). I. Photometric properties
• STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources
• SN 2016iet: The Pulsational or Pair Instability Explosion of a Low Metallicity Massive CO Core Embedded in a Dense Hydrogen-Poor Circumstellar Medium
• Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae
• Double Gravitational Wave Mergers
• Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers
• OGLE14-073 - a promising pair-instability supernova candidate
• Comment on "An excess of massive stars in the local 30 Doradus starburst"
• Twin LIGO/Virgo Detections of a Viable Gravitationally-Lensed Black Hole Merger

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