Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries

Keyphrases

• Binary Black Holes 100%
• Chemically Homogeneous Evolution 100%
• Binary Evolution 66%
• Merger Rate 66%
• Common Envelope 66%
• Monte Carlo Simulation 33%
• Theoretical Uncertainties 33%
• Tight 33%
• High-redshift 33%
• Helium 33%
• Total Mass 33%
• Gravitational Wave Detectors 33%
• Expected Rate 33%
• Dense Clusters 33%
• Chemical Gradient 33%
• Dynamical Interaction 33%
• Black Hole Mergers 33%
• Evolution Path 33%
• Hydrogen Burning 33%
• Equal Mass 33%
• Cosmic Time 33%
• Evolution Scenarios 33%
• Default Models 33%
• Local Binary 33%
• Short Time Delay 33%

Physics

• Black Hole 100%
• Monte Carlo Method 33%
• Gravitational Wave Detectors 33%
• Black Hole Merger 33%
• Hydrogen Burning 33%
• Stellar Envelope 33%