Black hole-naked singularity dualism and the repulsion of two Kerr black holes due to spin-spin interaction

DOI10.1016/j.physletb.2019.02.025zbMath1411.83067arXiv1803.03301OpenAlexW2789912161WikidataQ128352999 ScholiaQ128352999MaRDI QIDQ1738762

V. S. Man'ko, Eduardo Ruiz

Publication date: 18 April 2019

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1803.03301

zbMATH Keywords

naked singularitydouble-Kerr solutionbinary black holespin-spin interaction

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75)

Related Items (3)

Metric for two arbitrary Kerr sources ⋮ Binary systems of recoiling extreme Kerr black holes ⋮ Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities

Cites Work

• On the simplest binary system of stationary black holes
• Exact solution of the double-Kerr equilibrium problem
• Remarks on the Double-Kerr-Solution
• Exact event horizon of a black hole merger
• On a Simple Representation of the Kinnersley-Chitre Metric
• On rotating black holes in equilibrium in general relativity
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• On the Force Between Rotating Coaxial Black Holes
• Can test fields destroy the event horizon in the Kerr–Taub–NUT spacetime?
• Kerr–Newman black holes cannot be over-charged or over-spun

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