Instability of generalised AdS black holes and thermal field theory

TL;DR

This paper investigates the classical stability of generalized AdS black holes with arbitrary Einstein horizon metrics, revealing conditions for instability and their dual thermal field theory implications.

Contribution

It introduces a criterion for classical instability of AdS black holes with arbitrary horizons and explores the dual field theory interpretation via AdS/CFT correspondence.

Findings

Large black holes with B"ohm horizons can be unstable.

Unstable black holes can be thermodynamically stable.

Instability corresponds to a critical temperature in the dual field theory.

Abstract

We study black holes in AdS-like spacetimes, with the horizon given by an arbitrary positive curvature Einstein metric. A criterion for classical instability of such black holes is found in the large and small black hole limits. Examples of large unstable black holes have a B\"ohm metric as the horizon. These, classically unstable, large black holes are locally thermodynamically stable. The gravitational instability has a dual description, for example by using the $AdS_7 \times S^4$ version of the AdS/CFT correspondence. The instability corresponds to a critical temperature of the dual thermal field theory defined on a curved background.