Uniqueness theorem for charged rotating black holes in five-dimensional minimal supergravity

Journal Article · Mon Jun 15 00:00:00 EDT 2009 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.79.124023· OSTI ID:21300982

Tomizawa, Shinya; Ishibashi, Akihiro ^[1]; Yasui, Yukinori ^[2]

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1. Cosmophysics Group, Institute of Particle and Nuclear Studies, KEK, Tsukuba, Ibaraki, 305-0801 (Japan)
2. Department of Mathematics and Physics, Graduate School of Science, Osaka City University, 3-3-138 Sugimoto, Sumiyoshi, Osaka 558-8585 (Japan)

We show a uniqueness theorem for charged rotating black holes in the bosonic sector of five-dimensional minimal supergravity. More precisely, under the assumptions of the existence of two commuting axial isometries and spherical topology of horizon cross sections, we prove that an asymptotically flat, stationary charged rotating black hole with finite temperature in the five-dimensional Einstein-Maxwell-Chern-Simons theory is uniquely characterized by the mass, charge, and two independent angular momenta and therefore is described by the Chong-Cvetic-Lue-Pope solution. We also discuss a generalization of our uniqueness theorem for spherical black holes to the case of black rings.

• OSTI ID: 21300982
• Journal Information: Physical Review. D, Particles Fields, Vol. 79, Issue 12; Other Information: DOI: 10.1103/PhysRevD.79.124023; (c) 2009 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
ANGULAR MOMENTUM
BLACK HOLES
CROSS SECTIONS
EINSTEIN-MAXWELL EQUATIONS
MANY-DIMENSIONAL CALCULATIONS
MASS
MATHEMATICAL SOLUTIONS
SPHERICAL CONFIGURATION
SUPERGRAVITY