Does the Black Hole Merger Rate Evolve with Redshift?
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- Type
- article
- Published
- 2018-05-25
- Cited by
- 236
- References
- 48
- Access
- Open access
- OpenAlex
- https://openalex.org/W2804740880
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:118888624
Keywords
Redshift, Physics, Astrophysics, LIGO, Binary black hole
References
- NEUTRON STARS VERSUS BLACK HOLES: PROBING THE MASS GAP WITH LIGO/VIRGO
- Accounting for Source Uncertainties in Analyses of Astronomical Survey Data
- DOUBLE COMPACT OBJECTS. III. GRAVITATIONAL-WAVE DETECTION RATES
- The First Stellar Binary Black Holes: The Strongest Gravitational Wave Burst Sources
- On the Collapsar Model of Long Gamma-Ray Bursts:Constraints from Cosmic Metallicity Evolution
- DOUBLE COMPACT OBJECTS. I. THE SIGNIFICANCE OF THE COMMON ENVELOPE ON MERGER RATES
- The Nucleosynthetic Signature of Population III
- Probing Gravity with Spacetime Sirens
- The impact of star formation and gamma-ray burst rates at high redshift on cosmic chemical evolution and reionization
- Neutrino processes and pair formation in massive stars and supernovae.
- ON THE MASS DISTRIBUTION AND BIRTH MASSES OF NEUTRON STARS
- The concordance cosmic star formation rate: implications from and for the supernova neutrino and gamma ray backgrounds
- THE EFFECT OF METALLICITY ON THE DETECTION PROSPECTS FOR GRAVITATIONAL WAVES
- DOUBLE COMPACT OBJECTS. II. COSMOLOGICAL MERGER RATES
- The mass spectrum of compact remnants from the parsec stellar evolution tracks
- Possible indirect confirmation of the existence of Pop III massive stars by gravitational wave
- DISTINGUISHING COMPACT BINARY POPULATION SYNTHESIS MODELS USING GRAVITATIONAL WAVE OBSERVATIONS OF COALESCING BINARY BLACK HOLES
- Dynamics of stellar black holes in young star clusters with different metallicities – I. Implications for X-ray binaries
- Planck 2015 results: XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
- Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
Cited by
- Gravitational waves from the remnants of the first stars in nuclear star clusters
- Imprints of the redshift evolution of double neutron star merger rate on the signal-to-noise ratio distribution
- Black hole demography at the dawn of gravitational-wave astronomy: state-of-the art and future perspectives
- Black Hole Mergers from an Evolving Population of Globular Clusters.
- Cosmological impact of future constraints on H0 from gravitational-wave standard sirens
- Mining gravitational-wave catalogs to understand binary stellar evolution: A new hierarchical Bayesian framework
- Measuring the Star Formation Rate with Gravitational Waves from Binary Black Holes
- Redshift Evolution of the Black Hole Merger Rate from Globular Clusters
- An introduction to Bayesian inference in gravitational-wave astronomy: Parameter estimation, model selection, and hierarchical models
- Extracting distribution parameters from multiple uncertain observations with selection biases
- Stochastic Gravitational-wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
- Limits on Electromagnetic Counterparts of Gravitational-wave-detected Binary Black Hole Mergers
- The properties of merging black holes and neutron stars across cosmic time
- Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes.
- Distinguishing primordial black holes from astrophysical black holes by Einstein Telescope and Cosmic Explorer
- The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution
- Accuracy Requirements for Empirically Measured Selection Functions
- Parallelized inference for gravitational-wave astronomy
- Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers
- Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
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