Supersymmetric, Cold and Lukewarm Black Holes in Cosmological Einstein-maxwell Theory
نویسنده
چکیده
In flat space, the extreme Reissner-Nordstrøm (RN) black hole is distinguished by its coldness (vanishing Hawking temperature) and its supersymmetry. We examine RN solutions to Einstein-Maxwell theory with a cosmological constant Λ, classifying the cold black holes and, for positive Λ, the " lukewarm " black holes at the same temperature as the de Sitter thermal background. For negative Λ, we classify the supersymmetric solutions within the context of N = 2 gauged supergravity. One finds supersymmetric analogues of flat-space extreme RN black holes, which for nonzero Λ differ from the cold black holes. In addition, there is an exotic class of supersymmetric solutions which cannot be continued to flat space, since the magnetic charge becomes infinite in that limit.
منابع مشابه
Action and entropy of lukewarm black holes
We calculate the Euclidean actions and the entropies of lukewarm black holes, cold black holes and ultracold solutions in the Einstein-Maxwell theory with a positive cosmological constant. We find that the entropy of lukewarm black holes is sum of entropies of black hole horizon and cosmological horizon. The entropy of cold black holes is only one quarter area of cosmological horizon, and the e...
متن کاملUniqueness of near-horizon geometries of rotating extremal AdS4 black holes
We consider stationary extremal black hole solutions of the Einstein-Maxwell equations with a negative cosmological constant in four dimensions. We determine all non-static axisymmetric near-horizon geometries and all static near-horizon geometries for black holes of this kind. This allows us to deduce that the most general near-horizon geometry of an asymptotically globally AdS4 rotating extre...
متن کاملCharged Rotating Black Holes in 5d Einstein-Maxwell-(A)dS Gravity
We obtain charged rotating black hole solutions to the theory of Einstein-Maxwell gravity with cosmological constant in five dimensions. Some of the physical properties of these black holes are discussed. ∗email: [email protected] †email: [email protected]
متن کاملEinstein-Maxwell-Chern-Simons Black Holes
5-dimensional Einstein-Maxwell-Chern-Simons theory with Chern-Simons coefficient λ = 1 has supersymmetric black holes with vanishing horizon angular velocity, but finite angular momentum. Here supersymmetry is associated with a borderline between stability and instability, since for λ > 1 a rotational instability arises, where counterrotating black holes appear, whose horizon rotates in the opp...
متن کاملTopological black holes in the dimensionally continued gravity
We investigate the topological black holes in a special class of Lovelock gravity. In the odd dimensions, the action is the Chern-Simons form for the anti-de Sitter group. In the even dimensions, it is the Euler density constructed with the Lorentz part of the anti-de Sitter curvature tensor. The Lovelock coefficients are reduced to two independent parameters: cosmological constant and gravitat...
متن کامل