Non-existence of stationary two-black-hole configurations
J\"org Hennig, Gernot Neugebauer

TL;DR
This paper proves that two aligned sub-extremal black holes cannot be in a stationary equilibrium due to the incompatibility of their physical constraints, resolving a longstanding question in black hole physics.
Contribution
The authors formulate a boundary value problem and use inverse scattering methods to demonstrate the non-existence of stationary two-black-hole configurations.
Findings
No stationary equilibrium configurations exist for two aligned sub-extremal black holes.
Universal inequality between angular momentum and horizon area is key to the proof.
The result rules out the possibility of balanced two-black-hole systems in this setting.
Abstract
We resume former discussions of the question, whether the spin-spin repulsion and the gravitational attraction of two aligned sub-extremal black holes can balance each other. To answer the question we formulate a boundary value problem for two separate (Killing-) horizons and apply the inverse (scattering) method to solve it. Making use of a universal inequality between angular momentum and horizon area that has to be satisfied by every sub-extremal black hole, we prove the non-existence of the equilibrium situation in question.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Astrophysical Phenomena and Observations · Cosmology and Gravitation Theories
