black hole

black hole

UIB Binary Black Hole Merger, q=2, Seff=-0.35: lapse + orbital evolution

3h ago
SOURCE  

Description

Simulation of the first orbits of the lapse and orbital evolution of a mass ratio 2. with spins components {(0,0,-0.5)(0,0,-0.5)} of the dimensionless Kerr parameter. Visualization by Rafel Jaume Amengual, numerical simulation performed by Xisco Jiménez and Sascha Husa with the BAM code.