Abstract

We study nonminimal extensions of Einstein-Maxwell theory with exact electromagnetic duality invariance. Any such theory involves an infinite tower of higher-derivative terms whose computation and summation usually represents a challenging problem. Despite that, we manage to obtain a closed form of the action for all the theories with a quadratic dependence on the vector field strength. In these theories we find that the Maxwell field couples to gravity through a curvature-dependent susceptibility tensor that takes a peculiar form, reminiscent of that of Born-Infeld Lagrangians. We study the static and spherically symmetric black hole solutions of the simplest of these models, showing that the corresponding equations of motion are invariant under rotations of the electric and magnetic charges. We compute the perturbative corrections to the Reissner-Nordstr\"om solution in this theory, and in the case of extremal black holes we determine exactly the near-horizon geometry as well as the entropy. Remarkably, the entropy only possesses a constant correction despite the action containing an infinite number of terms. In addition, we find there is a lower bound for the charge and the mass of extremal black holes. When the sign of the coupling is such that the weak gravity conjecture is satisfied, the area and the entropy of extremal black holes vanish at the minimal charge.

Highlights

  • Symmetries are a powerful guide to constrain the possible corrections to low-energy effective actions

  • We study the static and spherically symmetric black hole solutions of the simplest of these models, showing that the corresponding equations of motion are invariant under rotations of the electric and magnetic charges

  • In this paper we have provided the first example of exactly duality-invariant theories with nonminimal couplings

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Summary

INTRODUCTION

Symmetries are a powerful guide to constrain the possible corrections to low-energy effective actions. One aspect of electromagnetic duality that distinguishes it from usual symmetries and that makes it interesting is the fact that it is nonlinear This means that, unlike in the case of linearly realized symmetries, one cannot find a basis of duality-invariant operators. Such extensions only preserve duality to leading order in α; in order to restore duality as an exact symmetry one needs to include an infinite tower of additional higher-derivative terms. In the case of the term TμνTμν, the simplest dualityinvariant completion corresponds to (Einstein-)Born-Infeld theory [10,11,12], a model that has been known for a long time and which is a paradigmatic example of a nonlinear duality-invariant theory—see [13,14,15,16,17,18,19,20,21,22] for other nonlinear models. The goal of this paper is to fill this gap, and we do so by studying the simplest duality-invariant completion of the Lagrangian RμνTμν

QUADRATIC THEORIES
STATIC AND SPHERICALLY SYMMETRIC CONFIGURATIONS
EXTREMAL BLACK HOLES AND NEAR-HORIZON GEOMETRIES
DISCUSSION
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