Five-dimensional gauged supergravity black holes with independent rotation parameters
Creators
- 1. George P. and Cynthia W. Mitchell Institute for Fundamental Physics, Texas A and M University, College Station, Texas 77843 (United States)
- 2. Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104 (United States)
Description
We construct new nonextremal rotating black hole solutions in SO(6) gauged five-dimensional supergravity. Our solutions are the first such examples in which the two rotation parameters are independently specifiable, rather than being set equal. The black holes carry charges for all three of the gauge fields in the U(1)3 subgroup of SO(6), albeit with only one independent charge parameter. We discuss the BPS limits, showing that these include the first examples of regular supersymmetric black holes with independent angular momenta in gauged supergravity. We also find nonsingular BPS solitons. Finally, we obtain another independent class of new rotating nonextremal black hole solutions with just one nonvanishing rotation parameter, and one nonvanishing charge
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.72.041901;
- arXiv
- arXiv:hep-th/0505112v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 72
- Journal Issue
- 4
- Journal Page Range
- p. 041901-041901.5
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37025663
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ANGULAR MOMENTUM; BLACK HOLES; MATHEMATICAL SOLUTIONS; QUANTUM FIELD THEORY; ROTATION; SO-6 GROUPS; SOLITONS; SUPERGRAVITY; SUPERSYMMETRY; U-1 GROUPS; UNITARY SYMMETRY
- Descriptors DEC
- FIELD THEORIES; LIE GROUPS; MOTION; QUASI PARTICLES; SO GROUPS; SYMMETRY; SYMMETRY GROUPS; U GROUPS; UNIFIED-FIELD THEORIES
Optional Information
- Notes
- (c) 2005 The American Physical Society