Stability of Horava-Lifshitz Black Holes in the Context of AdS/CFT

TL;DR

This paper investigates the stability of Hořava-Lifshitz black holes within the AdS/CFT framework, revealing conditions under which these black holes are stable or unstable, with implications for holographic superconductors.

Contribution

It provides the first detailed analysis of the stringy stability of Hořava-Lifshitz black holes in the context of AdS/CFT, highlighting stability conditions based on charge, curvature, and parameters.

Findings

Uncharged topological black holes in λ=1 Hořava-Lifshitz theory are nonperturbatively stable.

Certain charged black holes with specific parameters are unstable.

Implications for holographic superconductor models are discussed.

Abstract

The anti--de Sitter/conformal field theory (AdS/CFT) correspondence is a powerful tool that promises to provide new insights toward a full understanding of field theories under extreme conditions, including but not limited to quark-gluon plasma, Fermi liquid and superconductor. In many such applications, one typically models the field theory with asymptotically AdS black holes. These black holes are subjected to stringy effects that might render them unstable. Ho\v{r}ava-Lifshitz gravity, in which space and time undergo different transformations, has attracted attentions due to its power-counting renormalizability. In terms of AdS/CFT correspondence, Ho\v{r}ava-Lifshitz black holes might be useful to model holographic superconductors with Lifshitz scaling symmetry. It is thus interesting to study the stringy stability of Ho\v{r}ava-Lifshitz black holes in the context of AdS/CFT. We find that uncharged topological black holes in $\lambda=1$ Ho\v{r}ava-Lifshitz theory are nonperturbatively stable, unlike their counterparts in Einstein gravity, with the possible exceptions of negatively curved black holes with detailed balance parameter $\epsilon$ close to unity. Sufficiently charged flat black holes for $\epsilon$ close to unity, and sufficiently charged positively curved black holes with $\epsilon$ close to zero, are also unstable. The implication to the Ho\v{r}ava-Lifshitz holographic superconductor is discussed.