Multi-Black-Holes in Three Dimensions
arXiv:gr-qc/9402013 · doi:10.1103/PhysRevD.50.R7119
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.
8 pages, \LaTex, 4 figures (available on request), GCR 94/02/01
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