Warped AdS$_3$ black hole thermodynamics and the charged Cardy formula

TL;DR

This paper analyzes the thermodynamics of warped AdS$_3$ black holes in topologically massive gravity, linking gravitational properties to the charged Cardy formula and revealing unique features of the dual warped CFT$_2$.

Contribution

It introduces a method to express gravitational on-shell actions in the grand-canonical ensemble and clarifies the thermodynamic behavior of warped CFT$_2$, highlighting differences from previous studies.

Findings

The right-moving sector follows the charged Cardy formula.

The dual theory has a frozen left-moving state with non-zero entropy.

The approach clarifies the thermodynamic structure of warped CFTs.

Abstract

We revisit the thermodynamic properties of black holes with warped AdS$_3$ asymptotics in topologically massive gravity. The holographically dual theory, often referred to as warped CFT$_2$, exhibits a single copy of the Virasoro-Kac-Moody algebra. Consequently, the asymptotic density of states in the right-moving sector is described by the charged Cardy formula that we review in detail. By defining specific linear combinations of the gravitational thermodynamic potentials, we are able to present the gravitational left- and right-moving on-shell actions directly in the grand-canonical ensemble. This allows us to demonstrate that, apart from the charged Cardy behavior in the right-moving sector, the dual field theory exhibits an additional frozen left-moving state giving rise to non-zero entropy contribution. Our findings elucidate the nature of warped CFTs and reveal subtle yet fundamental differences from the existing literature.