Erratum to `Instability in cosmological topologically massive gravity at the chiral point', arXiv:0805.2610

Abstract

We correct a sign in the first variation of the on-shell action of cosmological topologically massive gravity at the chiral point and present the three equations affected by that sign. While this does not change any of the main conclusions of arXiv:0805.2610, it modifies the finite part of the Brown-York stress tensor. Our corrected Brown-York stress tensor is still finite, conserved and traceless, but no longer coincides with that of global AdS_3. It agrees with results found in recent literature.

2 pages, erratum to arXiv:0805.2610

References in corpus (2)

• Asymptotically anti-de Sitter spacetimes in topologically massive gravity
• Canonical analysis of cosmological topologically massive gravity at the chiral point

Cited by in corpus (5)

• Topologically Massive Gravity and the AdS/CFT Correspondence
• Boundary conditions for spacelike and timelike warped AdS_3 spaces in topologically massive gravity
• Asymptotically anti-de Sitter spacetimes in topologically massive gravity
• The CFT-interpolating Black Hole in Three Dimensions
• Topologically massive gravity on AdS${}_2$ spacetimes