Accuracy of inference on the physics of binary evolution from gravitational-wave observations

Abstract

The properties of the population of merging binary black holes encode some of the uncertain physics of the evolution of massive stars in binaries. The binary black hole merger rate and chirp mass distribution are being measured by ground-based gravitational-wave detectors. We consider isolated binary evolution and explore how accurately the physical model can be constrained with such observations by applying the Fisher information matrix to the merging black hole population simulated with the rapid binary population synthesis code COMPAS. We investigate variations in four COMPAS parameters: common envelope efficiency, kick velocity dispersion, and mass loss rates during the luminous blue variable and Wolf--Rayet stellar evolutionary phases. We find that 1000 observations would constrain these model parameters to a fractional accuracy of a few percent. Given the empirically determined binary black hole merger rate, we can expect gravitational-wave observations alone to place strong constraints on the physics of stellar and binary evolution within a few years.

12 pages, 9 figures; version accepted by Monthly Notices of the Royal Astronomical Society

References in corpus (21)

• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Cosmic Star Formation History
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Binary interaction dominates the evolution of massive stars
• GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
• Physical Properties of Wolf-Rayet Stars
• Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
• Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
• The Evolution of Compact Binary Star Systems
• Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• The impact of companions on stellar evolution
• Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
• Towards a better understanding of the evolution of Wolf-Rayet stars and Type Ib/Ic supernova progenitors
• The Impact of Star Formation and Gamma-Ray Burst Rates at High Redshift on Cosmic Chemical Evolution and Reionization
• The Galactic distribution of X-ray binaries and its implications for compact object formation and natal kicks
• LISA extreme-mass-ratio inspiral events as probes of the black hole mass function
• Model-independent inference on compact-binary observations
• Distinguishing types of compact-object binaries using the gravitational-wave signatures of their mergers
• A new prescription for the mass-loss rates of WC and WO stars
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo

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• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog
• The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range
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• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Gravitational Waves from Supernova Mass Loss and Natal Kicks in Close Binaries
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• The effect of redshift degeneracy and the damping effect of viscous medium on the information extracted from gravitational wave signals
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
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