THE EFFECT OF METALLICITY ON THE DETECTION PROSPECTS FOR GRAVITATIONAL WAVES
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- Type
- article
- Published
- 2010-04-02
- Cited by
- 208
- References
- 30
- Access
- Open access
- OpenAlex
- https://openalex.org/W2084955838
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:118394957
Keywords
Metallicity, Physics, Astrophysics, LIGO, Gravitational wave
References
- Formation of a Black Hole in the Dark
- On the Rarity of Double Black Hole Binaries: Consequences for Gravitational Wave Detection
- Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
- Mass loss and the evolution of massive stars
- The Orbital Period of the Wolf-Rayet Binary IC 10 X-1: Dynamic Evidence that the Compact Object Is a Black Hole
- A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
- Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors
- The Neutron star and black hole initial mass function
- A high-sensitivity pulsar survey
- The Total Merger Rate of Compact Object Binaries in the Local Universe
- Constraining Population Synthesis Models via Empirical Binary Compact Object Merger and Supernova Rates
- Compact Object Modeling with the StarTrack Population Synthesis Code
- The cosmic evolution of metallicity from the SDSS fossil record
- Supernova kicks and misaligned microquasars
- Double white dwarfs as progenitors of R Coronae Borealis stars and type I supernovae
- Thermal Timescale Mass Transfer and the Evolution of White Dwarf Binaries
- ON THE MAXIMUM MASS OF STELLAR BLACK HOLES
- Models for Massive Stellar Populations with Rotation
- An upper limit on the stochastic gravitational-wave background of cosmological origin
- IC10 X-1/NGC300 X-1: THE VERY IMMEDIATE PROGENITORS OF BH–BH BINARIES
Cited by
- Digging Deeper: Observing Primordial Gravitational Waves below the Binary-Black-Hole-Produced Stochastic Background.
- The neutron-star equation of state and gravitational waves from compact binaries
- The search for gravitational waves from the coalescence of black hole binary systems in data from the LIGO and Virgo detectors. Or: A dark walk through a random forest
- On the formation and evolution of the first Be star in a black hole binary MWC 656
- THE FATE OF Cyg X-1: AN EMPIRICAL LOWER LIMIT ON BLACK-HOLE–NEUTRON-STAR MERGER RATE
- DOUBLE COMPACT OBJECTS. III. GRAVITATIONAL-WAVE DETECTION RATES
- RELATIVISTIC SIMULATIONS OF BLACK HOLE–NEUTRON STAR COALESCENCE: THE JET EMERGES
- DOUBLE COMPACT OBJECTS AS LOW-FREQUENCY GRAVITATIONAL WAVE SOURCES
- PopCORN: Hunting down the differences between binary population synthesis codes
- Scientific objectives of Einstein Telescope
- Black hole-neutron star mergers in globular clusters
- Quasinormal modes of black holes: From astrophysics to string theory
- Effect of metallicity on the gravitational-wave signal from the cosmological population of compact binary coalescences
- A DEEP CHANDRA OBSERVATION OF THE WOLF–RAYET + BLACK HOLE BINARY NGC 300 X-1
- DOUBLE COMPACT OBJECTS. I. THE SIGNIFICANCE OF THE COMMON ENVELOPE ON MERGER RATES
- Low-frequency terrestrial gravitational-wave detectors
- THE BLACK HOLE FORMATION PROBABILITY
- Eccentric black hole-neutron star mergers: effects of black hole spin and equation of state
- Relativistic Binaries in Globular Clusters
- COMPACT OBJECT COALESCENCE RATE ESTIMATION FROM SHORT GAMMA-RAY BURST OBSERVATIONS
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