Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
arXiv:1906.04197 · doi:10.1103/PhysRevD.100.064060
Abstract
Using simulations performed with the population synthesis code MOBSE, we compute the merger rate densities and detection rates of compact binary mergers formed in isolation for second- and third-generation gravitational-wave detectors. We estimate how rates are affected by uncertainties on key stellar-physics parameters, namely common envelope evolution and natal kicks. We estimate how future upgrades will increase the size of the available catalog of merger events, and we discuss features of the merger rate density that will become accessible with third-generation detectors.
arXiv comment9 pages, 4 figures, 2 tables Matches the published version
References in corpus (46)
- Planck 2015 results. XIII. Cosmological parameters
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- On the variation of the Initial Mass Function
- 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
- Evolution of binary stars and the effect of tides on binary populations
- A statistical study of 233 pulsar proper motions
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Common Envelope Evolution: Where we stand and how we can move forward
- 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
- Physics, Astrophysics and Cosmology with Gravitational Waves
- Gravitational-wave sensitivity curves
- Observing binary inspiral in gravitational radiation: One interferometer
- Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
- Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
- Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
- Double Compact Objects III: Gravitational Wave Detection Rates
- Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections
- 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
- Networks of gravitational wave detectors and three figures of merit
- Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
- Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
- Massive black hole binaries from runaway collisions: the impact of metallicity
- Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
- Gravitational Radiation Detection with Laser Interferometry
- Theoretical uncertainties of the type Ia supernova rate
- Merging black holes in young star clusters
- Stellar-mass black holes in star clusters: implications for gravitational wave radiation
- Does the Black Hole Merger Rate Evolve with Redshift?
- Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries
- Compact Binary Merger Rates: Comparison with LIGO/Virgo Upper Limits
- Spin orientations of merging black holes formed from the evolution of stellar binaries
- The cosmic merger rate of neutron stars and black holes
- The cosmic merger rate of stellar black hole binaries from the Illustris simulation
- Prospects for doubling the range of Advanced LIGO
- Identification of the Long-Sought Common-Envelope Events
- The properties of merging black holes and neutron stars across cosmic time
- Accuracy of inference on the physics of binary evolution from gravitational-wave observations
- The impact of electron-capture supernovae on merging double neutron stars
- Explaining LIGO's observations via isolated binary evolution with natal kicks
- Parameter estimation for binary black holes with networks of third generation gravitational-wave detectors
- Inferences about supernova physics from gravitational-wave measurements: GW151226 spin misalignment as an indicator of strong black-hole natal kicks
- On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution
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- The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries
- 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
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- Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
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- A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
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