On the Hamiltonian form of 3D massive gravity
  We present a "Chern-Simons-like" action for the "general massive gravity" model propagating two spin-2 modes with independent masses in three spacetime dimensions (3D), and we use it to find a simple Hamiltonian form of this model. The number of local degrees of freedom, determined by the dimension of the physical phase space, agrees with a linearized analysis except in some limits, in particular that yielding "new topologically massive gravity", which therefore suffers from a linearization instability. 
Olaf Hohm, Alasdair Routh, Paul K. Townsend, Baocheng Zhang
hep-th gr-qc