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Instantons, black holes and harmonic functions

TLDR
In this article, a class of five-dimensional Einstein-Maxwell type Lagrangians, which contains the bosonic Lagrangian of vector multiplets as a subclass, and preserves some features of supersymmetry, namely the existence of multi-centered black hole solutions and of attractor equations, was constructed.
Abstract
We find a class of five-dimensional Einstein-Maxwell type Lagrangians which contains the bosonic Lagrangians of vector multiplets as a subclass, and preserves some features of supersymmetry, namely the existence of multi-centered black hole solutions and of attractor equations. Solutions can be expressed in terms of harmonic functions through a set of algebraic equations. The geometry underlying these Lagrangians is characterized by the existence of a Hesse potential and generalizes the very special real geometry of vector multiplets. Our construction proceeds by first obtaining instanton solutions for a class of four-dimensional Euclidean sigma models, which includes those occuring for four-dimensional Euclidean N=2 vector multiplets as a subclass.

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Journal ArticleDOI

Nonextremal black holes in gauged supergravity and the real formulation of special geometry

TL;DR: In this article, the authors give a rather general recipe for constructing nonextremal black hole solutions to the problem of supergravity coupled to abelian vector multiplets, using the formalism developed in [1], based on dimensional reduction and real formulation of special geometry.
Journal ArticleDOI

The Hesse potential, the c-map and black hole solutions

TL;DR: In this article, a new formulation of the local c-map is presented, which makes use of a symplectically covariant real formulation of special Kahler geometry. But this formulation is restricted to a class of prepotentials, which includes the very special (cubic) prepotsentials as a subclass.
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H-FGK formalism for black-hole solutions of N=2, d=4 and d=5 supergravity

TL;DR: In this paper, the Ferrara-Gibbons-Kallosh (FGK) black-hole effective action of N = 2, d = 4, 5 supergravities coupled to vector multiplets, replacing the metric warp factor and the physical scalars with real variables that transform in the same way as the charges under duality transformations.
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Nonextremal black holes in gauged supergravity and the real formulation of special geometry II

TL;DR: In this paper, a new prescription for finding nonextremal black hole solutions to N=2, D=4 Fayet-Iliopoulos gauged supergravity was presented, and explicit solutions of various models containing one vector multiplet were constructed.
Journal ArticleDOI

Non-extremal black holes, harmonic functions and attractor equations

TL;DR: In this paper, the authors presented a method to deform extremal black hole solutions into non-extremal solutions for a large class of supersymmetric and non-supersymmetric Einstein-vector-scalar-type theories.
References
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Book

Differential Geometry, Lie Groups, and Symmetric Spaces

TL;DR: In this article, the structure of semisimplepleasure Lie groups and Lie algebras is studied. But the classification of simple Lie algesbras and of symmetric spaces is left open.
Journal ArticleDOI

N=2 extremal black holes.

TL;DR: It is shown that extremal magnetic black hole solutions of N=2 supergravity coupled to vector multiplets with a generic holomorphic prepotential F can be described as supersymmetric solitons which interpolate between maximally symmetric limiting solutions at spatial infinity and the horizon.
Journal ArticleDOI

Supersymmetry and attractors.

TL;DR: The results provide an explicit model-independent expression for the macroscopic Bekenstein-Hawking entropy of {ital N}=2 black holes which is manifestly duality invariant.
Journal ArticleDOI

Schwarzschild field in n dimensions and the dimensionality of space problem

TL;DR: In this paper, it was shown that the bound state postulate uniquely entails the spatial dimensionality of geodesic equations of motion obtained from a generalization of the Schwarzschild field to static systems with hyperspherical symmetry.
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