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• W2042188945 startingPage "R4133" @default.
• W2042188945 abstract "Generalizations of the black hole geometry of Ba~nados, Teitelboim, and Zanelli (BTZ) are presented. The theory is three-dimensional vacuum Einstein theory with a negative cosmological constant. The $n$-black-hole solution has $n$ asymptotically anti-de Sitter exterior regions that join in one interior region. The geometry of each exterior region is identical to that of a BTZ geometry; in particular, each contains a black hole horizon that surrounds (as judged from that exterior) all the other horizons. The interior region acts as a closed universe containing $n$ black holes. The initial state and its time development are discussed in some detail for the simple case when the angular momentum parameters of all the black holes vanish. A procedure to construct $n$ black holes with angular momentum (for $n>~4$) is also given." @default.
• W2042188945 created "2016-06-24" @default.
• W2042188945 creator A5034426023 @default.
• W2042188945 date "1996-04-15" @default.
• W2042188945 modified "2023-10-18" @default.
• W2042188945 title "Multi-black-hole geometries in (2+1)-dimensional gravity" @default.
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• W2042188945 doi "https://doi.org/10.1103/physrevd.53.r4133" @default.
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