Three-dimensional black holes with conformally coupled scalar and gauge fields

TL;DR

This paper constructs and analyzes three-dimensional charged black holes with conformally coupled scalar and gauge fields, revealing unique thermodynamic properties and boundary conditions affecting their asymptotic symmetries.

Contribution

It introduces new black hole solutions with conformally coupled scalar and gauge fields in 3D gravity, exploring their thermodynamics and boundary conditions.

Findings

Black hole solutions are regular and asymptotically AdS.

Entropy does not follow the area law due to nonminimal coupling.

Conditions for positive entropy relate to boundary conditions and conformal symmetry.

Abstract

We consider three-dimensional gravity with negative cosmological constant in the presence of a scalar and an Abelian gauge field. Both fields are conformally coupled to gravity, the scalar field through a nonminimal coupling with the curvature and the gauge field by means of a Lagrangian given by a power of the Maxwell one. A sixth-power self-interaction potential, which does not spoil conformal invariance is also included in the action. Using a circularly symmetric ansatz, we obtain black hole solutions dressed with the scalar and gauge fields, which are regular on and outside the event horizon. These charged hairy black holes are asymptotically anti-de Sitter spacetimes. The mass and the electric charge are computed by using the Regge-Teitelboim Hamiltonian approach. If both leading and subleading terms of the asymptotic condition of the scalar field are present, a boundary condition that functionally relates them is required for determining the mass. Since the asymptotic form of the scalar field solution is defined by two integration constants, the boundary condition may or may not respect the asymptotic conformal symmetry. An analysis of the temperature and entropy of these black holes is presented. The temperature is a monotonically increasing function of the horizon radius as expected for asymptotically anti-de Sitter black holes. However, restrictions on the parameters describing the black holes are found by requiring the entropy to be positive, which, given the nonminimal coupling considered here, does not follow the area law. Remarkably, the same conditions ensure that the conformally related solutions become black holes in the Einstein frame.