Charged rotating Kaluza-Klein black holes in five dimensions

Journal Article · Fri Feb 15 00:00:00 EST 2008 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.77.044040· OSTI ID:21039160

Nakagawa, Toshiharu; Ishihara, Hideki; Matsuno, Ken; Tomizawa, Shinya ^[1]

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1. Department of Mathematics and Physics, Graduate School of Science, Osaka City University, 3-3-138 Sugimoto, Sumiyoshi, Osaka 558-8585 (Japan)

We construct a new charged rotating Kaluza-Klein black hole solution in the five-dimensional Einstein-Maxwell theory with a Chern-Simon term. The features of the solutions are also investigated. The spacetime is asymptotically locally flat, i.e., it asymptotes to a twisted S{sup 1} bundle over the four-dimensional Minkowski spacetime. The solution describe a non-BPS black hole rotating in the direction of the extra dimension. The solutions have the limits to the supersymmetric black hole solutions, a new extreme non-BPS black hole solution and a new rotating non-BPS black hole solution with a constant twisted S{sup 1} fiber.

• OSTI ID: 21039160
• Journal Information: Physical Review. D, Particles Fields, Vol. 77, Issue 4; Other Information: DOI: 10.1103/PhysRevD.77.044040; (c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BLACK HOLES
COSMOLOGY
EINSTEIN-MAXWELL EQUATIONS
FOUR-DIMENSIONAL CALCULATIONS
KALUZA-KLEIN THEORY
MANY-DIMENSIONAL CALCULATIONS
MATHEMATICAL SOLUTIONS
MINKOWSKI SPACE
SPACE-TIME
SUPERSYMMETRY