Abstract

We study nearly extreme black holes with nearly AdS2 horizon geometry in various settings inspired by string theory. Our focus is on the scales of the nAdS2 region and their relation to microscopic theory. These scales are determined by a generalization of the attractor mechanism for extremal black holes and realized geometrically as the normal derivatives along the extremal attractor flow. In some cases the scales are equivalently determined by the charge dependence of the extremal attractor by itself. Our examples include near extreme black holes in D ≥ 4 dimensions, AdS boundary conditions, rotation, and 5D black holes on the non-BPS branch.

Highlights

  • The holographic correspondence between nearly AdS2 geometry and nearly CFT1’s [1,2,3] is not conformal

  • We study nearly extreme black holes with nearly AdS2 horizon geometry in various settings inspired by string theory

  • Both sides of the duality depend on a scale and for both it is natural to focus on effective quantum field theory near the IR

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Summary

Introduction

The holographic correspondence between nearly AdS2 geometry and nearly CFT1’s [1,2,3] is not conformal. The radial derivative probes the extremal geometry infinitesimally beyond the AdS2 horizon region This is satisfying from an effective quantum field theory point of view because this simple device realizes geometrically the determination of the IR scale by matching with the UV data embodied in the attractor flow (radial dependence). The extremal attractor mechanism determines the value of these scalars at the horizon in terms of black hole charges while the nAttractor mechanism gives a (complex) scale analogous to (1.3) for each scalar These other scales are the dimensionful couplings entering the boundary theory describing vector fields in nAdS2 [26,27,28].

A 4D setting
The extremal attractor mechanism
A nAttractor mechanism for near-extremal black holes
Near extremal black hole thermodynamics from radial derivatives
Higher dimensional black holes
The standard nAttractor mechanism
Detailed example
Black holes in AdS4
Veff 4 R2
Standard nAttractor mechanism
Example
Rotating black holes
The attractor mechanism for extremal black holes
BPS black holes
General extremal black holes
Time-like charge vectors and the BPS branch
Space-like charge vectors and the non-BPS branch
Discussion
Space-like solutions
C Deriving black hole solutions for “space-like” charge vectors
Full Text
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