Einstein-Maxwell-Chern-Simons Black Holes

Abstract

Black holes in 5-dimensional Einstein-Maxwell-Chern-Simons (EMCS) theory and their intriguing properties are discussed. For the special case of the CS coupling constant $\lambda ={\lambda }_{SG}$, as obtained from supergravity, a closed form solution is known for the rotating black holes. Beyond this supergravity value, the EMCS black hole solutions can e.g. exhibit nonuniqueness and form sequences of radially excited solutions. In the presence of a negative cosmological constant the black holes can possess an extra-parameter corresponding to a magnetic flux in addition to the mass, electric charge and angular momenta. This latter family of black holes possesses also a solitonic limit. Finally, a new class of squashed EMCS black hole solutions is discussed.

arXiv comment8 pages, 13 figures, Contribution to the Proceedings of the 3rd Karl Schwarzschild Meeting (Frankfurt, July 24-28, 2017)

References in corpus (15)

• Rotation and the AdS/CFT correspondence
• D--branes and Spinning Black Holes
• The General Kerr-de Sitter Metrics in All Dimensions
• General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity
• Classification of near-horizon geometries of extremal black holes
• Charged Kerr-de Sitter Black Holes in Five Dimensions
• D=5 Einstein-Maxwell-Chern-Simons Black Holes
• The gravity dual of supersymmetric gauge theories on a squashed $S^1\times S^3$
• Anti-de-Sitter regular electric multipoles: towards Einstein-Maxwell-AdS solitons
• Properties of rotating Einstein-Maxwell-Dilaton black holes in odd dimensions
• Radially excited rotating black holes in Einstein-Maxwell-Chern-Simons theory
• Sequences of extremal radially excited rotating black holes
• Static Einstein-Maxwell Magnetic Solitons and Black Holes in an Odd Dimensional AdS Spacetime
• AdS${}_5$ magnetized solutions in minimal gauged supergravity
• Angular momentum-area proportionality of extremal charged black holes in odd dimensions

Cited by in corpus (1)

• Charged and rotating boson stars in 5-dimensional Einstein-Maxwell(-Chern-Simons) theory