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

Keyphrases

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

INIS

• black holes 100%
• astrophysics 100%
• signals 30%
• coalescence 30%
• comparative evaluations 20%
• range 20%
• instability 20%
• spin 20%
• general relativity theory 20%
• yields 10%
• probability 10%
• vectors 10%
• prediction 10%
• approximations 10%
• wave forms 10%
• precession 10%
• physical properties 10%
• numerical solution 10%
• red shift 10%
• gravitational waves 10%
• supernovae 10%
• star clusters 10%
• galaxy nuclei 10%

Physics

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