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Rotating Kaluza-Klein Black Holes

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arxiv hep-th/9909102 v3 pith:DTNIWT4S submitted 1999-09-15 hep-th

classification hep-th
keywords blackboundholeskaluza-kleinrotatingstatestheoryangular
verification ladder T0 review T1 audit T2 compute T3 formal
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All regular four-dimensional black holes are constructed in the theory obtained by Kaluza-Klein reduction of five-dimensional Einstein gravity. They are interpreted in string theory as rotating bound states of D0- and D6-branes. Conservation of angular momentum is important for the stability of the bound states. The thermodynamics, the duality symmetries, and the near-horizon limit are explored.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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

    hep-th 2026-07 conditional novelty 6.0 of 10

    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|.

  2. Index saddle for the D1-D5-P black string and its decoupling limit

    hep-th 2026-06 unverdicted novelty 6.0 of 10

    Constructs index saddle for D1-D5-P black string via BPS limit and uplift, with decoupling to BTZ x S^3 computing CFT index.

  3. Spinning generalizations of Majumdar-Papapetrou multi-black hole spacetimes: light rings, lensing and shadows

    gr-qc 2025-02 conditional novelty 6.0 of 10

    For the Teo-Wan two-black-hole spacetime, light rings merge and annihilate in pairs, giving total counts of 4, 6, or 8, and the shadows mimic double-Kerr.

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