Two identical black holes, but rotating in opposite directions collide

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SUMMARY

The collision of two identical black holes rotating in opposite directions results in complex gravitational interactions. When their ergospheres overlap, they create a region where movement along the plane of rotation is severely restricted. The gravitational forces of the black holes do not cancel each other out; instead, they can lead to significant gravitational recoil, with velocities reaching up to 4000 km/s for maximally-rotating holes. This phenomenon is detailed in the study referenced as arXiv:0702133, which systematically examines the gravitational recoil of equal-mass binaries with anti-aligned spins.

PREREQUISITES
  • Understanding of black hole physics and general relativity
  • Familiarity with ergosphere concepts in rotating black holes
  • Knowledge of gravitational recoil and its implications in astrophysics
  • Basic grasp of orbital mechanics and spin dynamics
NEXT STEPS
  • Research the implications of ergosphere dynamics in rotating black holes
  • Study gravitational recoil in binary black hole systems
  • Examine the findings of arXiv:0702133 on anti-aligned spins
  • Explore the effects of black hole collisions on surrounding spacetime
USEFUL FOR

Astronomers, astrophysicists, and students interested in black hole dynamics, gravitational physics, and the study of cosmic events involving colliding black holes.

Greglar
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What would happen? Would the result be a non-rotating black hole? During their collision when their ergospheres overlap, would it generate an area where nothing could move in either direction along the plane of rotation? Also, since the force of their gravitational pull would be the same, would they cancel each other out? Like would particles in the overlapping event horizons no longer fall towards either black hole?
 
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Some places to start looking:
http://arxiv.org/abs/gr-qc/0701164
http://arxiv.org/abs/gr-qc/0702133
http://arxiv.org/abs/gr-qc/0702052
http://arxiv.org/abs/0708.3999
http://arxiv.org/abs/1011.3281

The second of those seems most relevant: "Here we report the first systematic study of gravitational recoil of equal-mass binaries with equal, but anti-aligned, spins parallel to the orbital plane. Such an orientation of the spins is expected to maximize the recoil. We find that recoil velocity (which is perpendicular to the orbital plane) varies sinusoidally with the angle that the initial spin directions make with the initial linear momenta of each hole and scales up to a maximum of ~4000 km/s for maximally-rotating holes."
 
Last edited:
Awesome thanks! A lot more stuff goes on then I was expecting haha
 

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