A rotating Kaluza–Klein black hole with squashed horizons

2006/05/31 by Tower Wang · 9 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #hep-th

paper · pdf · doi:10.1016/j.nuclphysb.2006.09.001

published as Nucl.Phys.B756:86-99,2006 · LaTeX file, 18 pages, minor corrections, accepted by Nuclear Physics B

arxiv created 2006/09/05 · openalex publication_date 2006/09/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We find a rotating Kaluza-Klein black hole solution with a squashed S³ horizon in five dimensions. This is a Kerr counterpart of the charged one found by Ishihara and Matsuno (hep-th/0510094) recently. The space-time is geodesic complete and free of naked singularity. Its asymptotic structure is a twisted S¹ fiber bundle over a four dimensional Minkowski space-time. We also study the mass and thermodynamics of this black hole.

Citations

• A Model for High Energy Scattering in Quantum Gravity
• Stability of gravity with a cosmological constant
• Conserved charges in even dimensional asymptotically locally anti-de Sitter space-times
• On the gravitational energy of the Kaluza–Klein monopole

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• Cosmological black holes on Taub–NUT space in five-dimensional Einstein–Maxwell theory
• Extremal Kerr/CFT correspondence of five-dimensional rotating (charged) black holes with squashed horizons
• Evolution of perturbations of squashed Kaluza-Klein black holes: Escape from instability
• Rotating Kaluza-Klein multi-black holes with Gödel parameter
• Rotating black ring on Kaluza-Klein bubbles
• X-ray reflection spectroscopy with Kaluza–Klein black holes