Properties and Astrophysical Implications of the 150 M _o˙Binary Black Hole Merger GW190521

Keyphrases

• Active Galactic nuclei 33%
• Binary Black Holes 66%
• Binary Merger 33%
• Black Hole Binaries 100%
• Black Hole Coalescence 33%
• Black Hole Mergers 100%
• Consistent Estimation 33%
• General Relativity 66%
• Gravitational Waves 33%
• Intermediate-mass Black Holes 33%
• Lensing 33%
• Low-mass 66%
• Mass Gap 66%
• Merger Rate 33%
• Numerical Solution 33%
• Orbital Precession 33%
• Pair Instability 33%
• Pair-instability Supernovae 33%
• Physical Properties 33%
• Possible Sources 33%
• Primordial Black Holes 33%
• Quasi-circular 33%
• Ringdown 33%
• Similar Systems 33%
• Spin Vector 33%
• Star Clusters 33%
• Stellar Collapse 33%
• Strong Field 33%
• Waveform Modeling 33%

Physics

• Active Galactic Nuclei 16%
• Black Hole 100%
• Black Hole Merger 100%
• General Relativity 33%
• Gravitational Wave 16%
• Intermediate-Mass Black Holes 16%
• Numerical Solution 16%
• Primordial Black Holes 16%
• Star Cluster 16%
• Supernovae 16%