Binary Black Holes

A rudimentary visualization of binary black hole merger. The simulation correspond to two non-spinning black holes of mass ratio 0.6. The location of the centres of these black holes are obtained directly from numerical simulations.

Visualization of the tidal deformation of dynamical horizons in a binary black hole merger scenario. This video shows that the dynamical horizons of even non-spinning black holes defrom. Please see visit the page on Generalized Deformations for more details.