Rates of Compact Object Coalescences

Abstract

Gravitational-wave detections are enabling measurements of the rate of coalescences of binaries composed of two compact objects -- neutron stars and/or black holes. The coalescence rate of binaries containing neutron stars is further constrained by electromagnetic observations, including Galactic radio binary pulsars and short gamma-ray bursts. Meanwhile, increasingly sophisticated models of compact objects merging through a variety of evolutionary channels produce a range of theoretically predicted rates. Rapid improvements in instrument sensitivity, along with plans for new and improved surveys, make this an opportune time to summarise the existing observational and theoretical knowledge of compact-binary coalescence rates.

arXiv commentInvited review article for Living Reviews in Relativity. Updates relative to published version based on recent observations and models. The authors very much welcome further suggestions. All code and data are publicly available via https://zenodo.org/record/7017532 (version 7)

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• Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
• Stochastic gravitational wave background due to gravitational wave memory
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors
• Thermonuclear and Electron-Capture Supernovae from Stripped-Envelope Stars
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• Effect of a High-Precision Semi-Analytical Mass Function on the Merger Rate of Primordial Black Holes in Dark Matter Halos
• Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
• Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Analytic Modelling of Binary-Single Encounters: Non-Thermal Eccentricity Distribution and Gravitational-Wave Source Formation
• Multi-messenger Emission from Tidal Waves in Neutron Star Oceans
• VFTS 243 as predicted by the BPASS fiducial models
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Formation of the First Two Black Hole-Neutron Star Mergers (GW200115 and GW200105) from Isolated Binary Evolution
• Velocity offset between emission and absorption lines might be an effective indicator of dual core system
• Rapid stellar and binary population synthesis with COMPAS
• Gravitational-wave bursts from spin-precessing black holes in binary systems
• Probing Formation of Double Neutron Star Binaries around 1mHz with LISA
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Gravitational wave astronomy: astrophysical and cosmological inferences
• Estimating Transient Rates from Cosmological Simulations and BPASS