Instability in cosmological topologically massive gravity at the chiral point

TL;DR

This paper investigates the instability caused by a negative energy mode in cosmological topologically massive gravity at the chiral point, analyzing its properties and implications for the theory's stability and chiral gravity prospects.

Contribution

It demonstrates the existence of a negative energy bulk mode, proves it is not pure gauge, and explores boundary conditions and holographic renormalization to assess stability.

Findings

Negative energy mode grows linearly in time

Mode is not pure gauge and has finite negative energy

Boundary conditions are compatible with asymptotically AdS_3

Abstract

We consider cosmological topologically massive gravity at the chiral point with positive sign of the Einstein-Hilbert term. We demonstrate the presence of a negative energy bulk mode that grows linearly in time. Unless there are physical reasons to discard this mode, this theory is unstable. To address this issue we prove that the mode is not pure gauge and that its negative energy is time-independent and finite. The isometry generators L_0 and \bar{L}_0 have non-unitary matrix representations like in logarithmic CFT. While the new mode obeys boundary conditions that are slightly weaker than the ones by Brown and Henneaux, its fall-off behavior is compatible with spacetime being asymptotically AdS_3. We employ holographic renormalization to show that the variational principle is well-defined. The corresponding Brown-York stress tensor is finite, traceless and conserved. Finally we address possibilities to eliminate the instability and prospects for chiral gravity.