Note on New Massive Gravity in
arXiv:0903.0536 · doi:10.1088/1126-6708/2009/04/106
Abstract
In this note we study the properties of linearized gravitational excitations in the new massive gravity theory in asymptotically spacetime and find that there is also a critical point for the mass parameter at which massive gravitons become massless as in topological massive gravity in . However, at this critical point in the new massive gravity the energy of all branches of highest weight gravitons vanish and the central charges also vanish within the Brown-Henneaux boundary conditions. The new massive gravity in asymptotically spacetime seems to be trivial at this critical point under the Brown-Henneaux boundary conditions if the Brown-Henneaux boundary conditions can be consistent with this theory. At this point, the boundary conditions of log gravity may be preferred.
v3 typos corrected, refs added, version to appear in JHEP
References in corpus (11)
- Massive Gravity in Three Dimensions
- Three-Dimensional Gravity Revisited
- Asymptotically anti-de Sitter spacetimes in topologically massive gravity
- Constraints on extremal self-dual CFTs
- Canonical structure of topologically massive gravity with a cosmological constant
- A Simple Proof of the Chiral Gravity Conjecture
- Canonical analysis of cosmological topologically massive gravity at the chiral point
- On Non-handlebody Instantons in 3D Gravity
- Comment on "Cosmological Topological Massive Gravitons and Photons"
- Partition Functions of Three-Dimensional Pure Gravity
- Monster symmetry and Extremal CFTs
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- Massive Gravity with Mass Term in Three Dimensions
- Kundt spacetimes of massive gravity in three dimensions
- Renormalizability of Topologically Massive Gravity