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A Double Myers-Perry Black Hole in Five Dimensions

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arxiv 0805.1206 v2 pith:ZOHBMLDN submitted 2008-05-08 hep-th

A Double Myers-Perry Black Hole in Five Dimensions

classification hep-th
keywords blackdimensionaldoubleholesmyers-perryarisingbackgroundconical
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Using the inverse scattering method we construct a six-parameter family of exact, stationary, asymptotically flat solutions of the 4+1 dimensional vacuum Einstein equations, with U(1)^2 rotational symmetry. It describes the superposition of two Myers-Perry black holes, each with a single angular momentum parameter, both in the same plane. The black holes live in a background geometry which is the Euclidean C-metric with an extra flat time direction. This background possesses conical singularities in two adjacent compact regions, each corresponding to a set of fixed points of one of the U(1) actions in the Cartan sub-algebra of SO(4). We discuss several aspects of the black holes geometry, including the conical singularities arising from force imbalance, and the torsion singularity arising from torque imbalance. The double Myers-Perry solution presented herein is considerably simpler than the four dimensional double Kerr solution and might be of interest in studying spin-spin interactions in five dimensional general relativity.

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  1. Multi-rotating black holes with non-aligned angular momenta in 5D Kaluza-Klein theory

    hep-th 2026-07 conditional novelty 6.0

    Exact multi-centered rotating dyonic black holes with non-aligned angular momenta exist in 5D KK theory and remain regular (no curvature singularities or CTCs) when |J_i| < |P_i Q_i|.