Abstract
Abstract: We have investigated the upper bound of the radiation energy in the head-on collision of two Myers-Perry black holes. Initially, the two black holes are far away from each other, and they become one black hole after the collision. We have obtained the upper bound of the radiation energy thermodynamically allowed in the process. The upper bound of the radiation energy is obtained in general dimensions. The radiation bound depends on the alignments of rotating axes for a given initial condition due to spin-spin interaction. We have found that the collision may not be occurred for a initially ultra-spinning black hole.
Original language | English |
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Article number | 79 |
Journal | Journal of High Energy Physics |
Volume | 2016 |
Issue number | 7 |
DOIs | |
State | Published - 1 Jul 2016 |
Keywords
- Black Holes
- Classical Theories of Gravity