Abstract
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/M0.95) and the radiated energy can be as large as 35±5% of the center-of-mass energy.
Original language | English (US) |
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Article number | 131102 |
Journal | Physical review letters |
Volume | 103 |
Issue number | 13 |
DOIs | |
State | Published - Sep 22 2009 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy