Zoom-whirl orbits occur for charged black hole binaries, and the merger and scattering thresholds become universal when normalized by the sum of irreducible masses.
These results demonstrate that zoom-whirl behavior can be exhibited for at least λ = 0 .6, and that the elec- trostatic repulsion does not suppress zoom-whirl orbits
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High-energy interactions of charged black holes in full general relativity I: Zoom-whirl orbits and universality with the irreducible mass
Zoom-whirl orbits occur for charged black hole binaries, and the merger and scattering thresholds become universal when normalized by the sum of irreducible masses.