Cross section, final spin and zoom-whirl behavior in high-energy black hole collisions

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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Rearranged results section; accepted for publication in Phys. Rev. Lett

Scientific paper

10.1103/PhysRevLett.103.131102

We study the collision of two highly boosted equal mass, nonrotating black holes with generic impact parameter. We find such systems to exhibit zoom-whirl behavior when fine tuning the impact parameter. Near the threshold of immediate merger the remnant black hole Kerr parameter can be near maximal (a/M about 0.95) and the radiated energy can be as large as 35% of the center-of-mass energy.

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