Initial Data for Black Holes and Black Strings in 5d
Evgeny Sorkin, Tsvi Piran

TL;DR
This paper investigates the topology change of apparent horizons in five-dimensional spacetimes with a compactified dimension, revealing a discontinuous phase transition between spherical and ring-like horizons.
Contribution
It introduces initial data for black objects in 5d with a compact dimension and identifies a novel phase transition in horizon topology.
Findings
Horizon topology changes from S^3 to S^2 x S^1
Discontinuous phase transition observed
Possible phase diagram proposed
Abstract
We explore time-symmetric hypersurfaces containing apparent horizons of black objects in a 5d spacetime with one coordinate compactified on a circle. We find a phase transition within the family of such hypersurfaces: the horizon has different topology for different parameters. The topology varies from to . This phase transition is discontinuous -- the topology of the horizon changes abruptly. We explore the behavior around the critical point and present a possible phase diagram.
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