Spinning Black Binaries in de Sitter space
General Relativity and Quantum Cosmology
2024-06-18 v1 High Energy Physics - Theory
Abstract
We construct stationary, rotating black binaries in general relativity with a positive cosmological constant. We consider identical black holes with either aligned or anti-aligned spins. Both cases have less entropy than the corresponding single Kerr/Schwarzschild de Sitter black hole with the same total angular momentum and cosmological horizon entropy. Our solutions establish continuous non-uniqueness in general relativity without matter. They also provide initial data for the spinning binary merger problem (when orbital angular momentum is added).
Cite
@article{arxiv.2406.10333,
title = {Spinning Black Binaries in de Sitter space},
author = {Oscar J. C. Dias and Jorge E. Santos and Benson Way},
journal= {arXiv preprint arXiv:2406.10333},
year = {2024}
}
Comments
15 pages, 11 figures. arXiv admin note: text overlap with arXiv:2303.07361