Multi-Black-Holes in Three Dimensions
General Relativity and Quantum Cosmology
2009-12-30 v1 High Energy Physics - Theory
Abstract
We construct time-dependent multi-centre solutions to three-dimensional general relativity with zero or negative cosmological constant. These solutions correspond to dynamical systems of freely falling black holes and conical singularities, with a multiply connected spacetime topology. Stationary multi-black-hole solutions are possible only in the extreme black hole case.
Cite
@article{arxiv.gr-qc/9402013,
title = {Multi-Black-Holes in Three Dimensions},
author = {Gérard Clément},
journal= {arXiv preprint arXiv:gr-qc/9402013},
year = {2009}
}
Comments
8 pages, \LaTex, 4 figures (available on request), GCR 94/02/01