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Kaluza-Klein Black Holes with Squashed Horizons

2005/10/31 by Hideki Ishihara, Ken Matsuno · 9 citations
Mathematics · Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Geometric Analysis and Curvature Flows #gr-qc #hep-th

paper · pdf · doi:10.1143/ptp.116.417

published as Prog.Theor.Phys. 116 (2006) 417-422 · 9pages. Final version to appear in Progress of Theoretical Physics

openalex publication_date 2006/08/01 · arxiv created 2006/08/08 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We study geometrical structures of charged static black holes in the five-dimensional Einstein-Maxwell theory. The black holes we study have horizons in the form of squashed S3, and their asymptotic structure consists of a twisted S1 bundle over the four-dimensional flat spacetime at the spatial infinity. The spacetime we consider is fully five-dimensional in the vicinity of the black hole and four-dimensional with a compact extra dimension at infinity.

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