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- W2008003954 abstract "We numerically study the event horizons of two kinds of five-dimensional coalescing black hole solutions with different asymptotic structures: the five-dimensional Kastor-Traschen solution (5DKT) and the coalescing black hole solution on Eguchi-Hanson space (CBEH). Topologies of the spatial infinity are ${rm S}^3$ and $L(2;1)={rm S}^3/{mathbb Z}_2$, respectively. We show that the crease sets of event horizons are topologically ${rm R}^1$ in 5DKT and ${rm R}^1times {rm S}^1$ in CBEH, respectively. If we choose the time slices which respect space-time symmetry, the first contact points of the coalescing process is a point in the 5DKT case but a ${rm S}^1$ in the CBEH case. We also find that in CBEH, time slices can be chosen so that a black ring with ${rm S}^1times {rm S}^2$ topology can be also formed during a certain intermediate period unlike the 5DKT." @default.
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- W2008003954 date "2009-09-21" @default.
- W2008003954 modified "2023-09-25" @default.
- W2008003954 title "Topology changing process of coalescing black holes on Eguchi-Hanson space" @default.
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- W2008003954 doi "https://doi.org/10.1103/physrevd.80.064030" @default.
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