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Multi-Black-Holes in 3D and 4D anti-de Sitter Spacetimes

Dieter R. Brill
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Abstract

The (single) black hole solutions of Bañados, Teitelboim and Zanelli (BTZ) in 2+1 dimensional anti-de Sitter space are generalized to an arbitrary number $n$ of such black holes. The resulting multi-black-hole (MBH) spacetime is locally isometric to anti-de Sitter space, and globally it is obtained from the latter as a quotient space by means of suitable identifications. The MBH spacetime has $n$ asymptotically anti-de Sitter exterior regions, each of which has the geometry of a single BTZ black hole. These exterior regions are separated by $n$ horizons from a common interior region. This interior region can be described as a ``closed" universe containing $n$ black holes. Similar configurations in 3+1 dimensions, with horizons of toroidal and higher genus topologies, are also presented.

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Dieter R. Brill. 1996-08-05. Multi-Black-Holes in 3D and 4D anti-de Sitter Spacetimes. https://arxiv.org/abs/gr-qc/9608010

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