Double Compact Objects III: Gravitational Wave Detection Rates

Abstract

The unprecedented range of second-generation gravitational-wave (GW) observatories calls for refining the predictions of potential sources and detection rates. The coalescence of double compact objects (DCOs)---i.e., neutron star-neutron star (NS-NS), black hole-neutron star (BH-NS), and black hole-black hole (BH-BH) binary systems---is the most promising source of GWs for these detectors. We compute detection rates of coalescing DCOs in second-generation GW detectors using the latest models for their cosmological evolution, and implementing inspiral-merger-ringdown (IMR) gravitational waveform models in our signal-to-noise ratio calculations. We find that: (1) the inclusion of the merger/ringdown portion of the signal does not significantly affect rates for NS-NS and BH-NS systems, but it boosts rates by a factor $\sim 1.5$ for BH-BH systems; (2) in almost all of our models BH-BH systems yield by far the largest rates, followed by NS-NS and BH-NS systems, respectively, and (3) a majority of the detectable BH-BH systems were formed in the early Universe in low-metallicity environments. We make predictions for the distributions of detected binaries and discuss what the first GW detections will teach us about the astrophysics underlying binary formation and evolution.

published in ApJ, 19 pages, 11 figures

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• Projections of the uncertainty on the compact binary population background using popstock
• Eccentricity matters: Impact of eccentricity on inferred binary black hole populations
• Mechanisms for high spin in black-hole neutron-star binaries and kilonova emission: inheritance and accretion
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• How close can we approach the event horizon of the Kerr black hole from the detection of the gravitational quasinormal modes?
• Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors
• Forecasting the population properties of merging black holes
• Propagation of gravitational waves in an expanding background in the presence of a point mass
• Measurement of Tidal Deformability in the Gravitational Wave Parameter Estimation for Nonspinning Binary Neutron Star Mergers
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Capability of Detecting Ultra-Violet Counterparts of Gravitational Waves with GLUV
• Efficiency of nonspinning templates in gravitational wave searches for aligned-spin binary black holes
• Blue Supergiant X-ray Binaries in the Nearby Dwarf Galaxy IC 10
• Recent LIGO-Virgo discoveries
• Using Galaxy Formation Simulations to optimise LIGO Follow-Up Observations
• Black Hole Merger Rates in AGN: contribution from gas-captured binaries
• Imprints of massive black-hole binaries on neighbouring decihertz gravitational-wave sources
• Extreme resonant eccentricity excitation of stars around merging black-hole binary
• Accuracy in Measuring the Neutron Star Mass in Gravitational Wave Parameter Estimation for Black Hole-Neutron Star Binaries
• Systematic Bias Due to Nonspinning Template Waveforms in the Gravitational Wave Parameter Estimation for Aligned-Spin Binary Black Holes
• Implications of binary black hole detections on the merger rates of double neutron stars and neutron star-black holes
• Comparing the birth rate of stellar black holes in binary black hole mergers and long GRBs
• Projected gravitational wave constraints on primordial black hole abundance for extended mass distributions
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Connecting Numerical Relativity and Data Analysis of Gravitational Wave Detectors
• Gravitational Waves and Electromagnetic Transients
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
• Primordial black holes with mass ratio-modulated initial clustering: merger suppression and projected constraints
• Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
• A Study of Systematics on the Cosmological Inference of the Hubble Constant from Gravitational Wave Standard Sirens
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• 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
• Inferring binary black holes stellar progenitors with gravitational wave sources