Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers
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- Type
- article
- Published
- 2019-05-29
- Cited by
- 80
- References
- 83
- Access
- Open access
- OpenAlex
- https://openalex.org/W2946945237
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:170078971
Keywords
Binary number, Pairing, Binary black hole, Mass ratio, Component (thermodynamics)
References
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- Advanced Virgo: a second-generation interferometric gravitational wave detector
- Binary inspiral, gravitational radiation, and cosmology.
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- Estimating the Size of a Population
- The Weighted Likelihood Ratio, Linear Hypotheses on Normal Location Parameters
- Exploring the consequences of pairing algorithms for binary stars
- Observing binary inspiral in gravitational radiation: One interferometer.
- Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
- Nuclear-powered millisecond pulsars and the maximum spin frequency of neutron stars
- DISTINGUISHING COMPACT BINARY POPULATION SYNTHESIS MODELS USING GRAVITATIONAL WAVE OBSERVATIONS OF COALESCING BINARY BLACK HOLES
- Characterization of the LIGO detectors during their sixth science run
- Planck 2015 results: XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
- Relativistic mergers of black hole binaries have large, similar masses, low spins and are circular
Cited by
- Supernovae in massive binaries and compact object mergers near supermassive black holes
- Merger Rate of Stellar Black Hole Binaries above the Pair-instability Mass Gap
- Black holes in the low-mass gap: Implications for gravitational-wave observations
- Black Hole Coagulation: Modeling Hierarchical Mergers in Black Hole Populations
- Primordial black hole merger rates: distributions for multiple LIGO observables
- Counting on Short Gamma-Ray Bursts: Gravitational-wave Constraints of Jet Geometry
- The Low Effective Spin of Binary Black Holes and Implications for Individual Gravitational-wave Events
- Merging Black Holes in the Low-mass and High-mass Gaps from 2 + 2 Quadruple Systems
- Endpoint of the up-down instability in precessing binary black holes
- Shouts and Murmurs: Combining Individual Gravitational-wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers
- 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
- Spin Evolution of Stellar-mass Black Hole Binaries in Active Galactic Nuclei
- Jumping the Gap: Searching for LIGO’s Biggest Black Holes
- Does Matter Matter? Using the Mass Distribution to Distinguish Neutron Stars and Black Holes
- Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass
- Primordial black holes from cusp collapse on cosmic strings
- Evaluating the merger rate of binary black holes from direct captures and third-body soft interactions using the Milky Way globular clusters
- New Spin on LIGO-Virgo Binary Black Holes.
- The Origin of Inequality: Isolated Formation of a 30+10 M ⊙ Binary Black Hole Merger
- A fixed point for black hole distributions
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