Exactly Soluble BPS Black Holes in Higher Curvature N=2 Supergravity

Abstract

We find a class of d=4, N=2 supergravity with $R^2$-interactions that admits exact BPS black holes. The prepotential contains quadratic, cubic and chiral curvature-squared terms. Black hole geometry realizes stretched horizon, and consists of anti-de Sitter, intermediate and outermost flat regions. Mass and entropy depends on charges and are modified not only by higher curvature terms but also by quadratic term in the prepotential. Consequently, even for large charges, entropy is no longer proportional to mass-squared.

arXiv comment4 pages, revtex4, 2 figures; v2. minor corrections

Cited by in corpus (24)

• Black Hole Entropy Function and the Attractor Mechanism in Higher Derivative Gravity
• Black Hole Entropy Function, Attractors and Precision Counting of Microstates
• Rotating Attractors
• Precision Counting of Small Black Holes
• Higher Derivative Corrections to Non-supersymmetric Extremal Black Holes in N=2 Supergravity
• Exploring the relation between 4D and 5D BPS solutions
• General 2 charge geometries
• Two Centered Black Holes and N=4 Dyon Spectrum
• Two Charge System Revisited: Small Black Holes or Horizonless Solutions?
• R^4 Corrections to D1D5p Black Hole Entropy from Entropy Function Formalism
• One entropy function to rule them all
• Supersymmetric black holes
• New attractor mechanism for spherically symmetric extremal black holes
• Extremal dyonic black holes in D=4 Gauss-Bonnet gravity
• Entropy of an extremal regular black hole
• All Higher Genus BPS Membranes in the Plane Wave Background
• The alpha-prime stretched horizon in the Heterotic string
• Global solutions for higher-dimensional stretched small black holes
• Entropy Function and Universality of Entropy-Area Relation for Small Black Holes
• Superconformal Quantum Mechanics of Small Black Holes
• Black Holes and the Spectrum of Half-BPS States in N=4 Supersymmetric String Theory
• Introduction to black hole entropy and supersymmetry
• Large Charge Four-Dimensional Extremal N=2 Black Holes with R^2-Terms
• Large Charge Four-Dimensional Non-Extremal N=2 Black Holes with R^2-Terms