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arXiv · gr-qc/9810080

Formation of a rotating hole from a close limit head-on collision

W. Krivan·R. H. Price
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Abstract

Realistic black hole collisions result in a rapidly rotating Kerr hole, but simulations to date have focused on nonrotating final holes. Using a new solution of the Einstein initial value equations we present here waveforms and radiation for an axisymmetric Kerr-hole-forming collision starting from small initial separation (the ``close limit'' approximation) of two identical rotating holes. Several new features are present in the results: (i) In the limit of small separation, the waveform is linear (not quadratic) in the separation. (ii) The waveforms show damped oscillations mixing quasinormal ringing of different multipoles.

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W. Krivan, R. H. Price. 1998-10-26. Formation of a rotating hole from a close limit head-on collision. https://doi.org/10.1103/physrevlett.82.1358

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