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No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
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Related Experiment Video

Updated: Jun 8, 2026

Automated Delivery of Microfabricated Targets for Intense Laser Irradiation Experiments
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Particle accelerators inside spinning black holes.

Kayll Lake1

  • 1Department of Physics, Queen's University, Kingston, Ontario, Canada, K7L 3N6. lake@astro.queensu.ca

Physical Review Letters
|September 28, 2010
PubMed
Summary
This summary is machine-generated.

Colliding particles near spinning black holes reveal an instability at the inner horizon. This suggests that Planck-scale physics is relevant within black holes, even at larger scales.

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Area of Science:

  • Astrophysics
  • General Relativity
  • Black Hole Physics

Background:

  • The Kerr metric describes rotating black holes.
  • Previous studies identified Cauchy horizon instability in black holes.

Purpose of the Study:

  • To investigate the center-of-mass energy of colliding particles near a spinning black hole.
  • To determine the stability of classical black holes.

Main Methods:

  • Utilizing the Kerr metric to model a spinning black hole accreting test particles.
  • Analyzing the behavior of particle collisions at the inner horizon.

Main Results:

  • The center-of-mass energy diverges at the inner horizon for rotating black holes.
  • This divergence is unique to rotating black holes and distinct from Cauchy horizon instability.
  • The findings imply that Planck-scale physics is relevant within black holes at larger scales.

Conclusions:

  • Classical black holes with rotation are internally unstable.
  • Black hole interiors may exhibit Planck-scale physics at accessible scales.
  • The discovered instability highlights a novel aspect of black hole dynamics.