Bending AdS waves with new massive gravity

We study AdS-waves in the three-dimensional new theory of massive gravity recently proposed by Bergshoeff, Hohm, and Townsend. The general configuration of this type is derived and shown to exhibit different branches, with different asymptotic behaviors. In particular, for the special fine tuning m² = ±1/(2l²), solutions with logarithmic fall-off arise, while in the range m² > -1/(2l²), spacetimes with Schrödinger isometry group are admitted as solutions. Spacetimes that are asymptotically AdS₃, both for the Brown-Henneaux and for the weakened boundary conditions, are also identified. The metric function that characterizes the profile of the AdS-wave behaves as a massive excitation on the spacetime, with an effective mass given by m_eff² = m²-1/(2l²). For the critical value m² = -1/(2l²), the value of the effective mass precisely saturates the Breitenlohner-Freedman bound for the AdS₃ space where the wave is propagating on. The analogies with the AdS-wave solutions of topologically massive gravity are also discussed. Besides, we consider the coupling of both massive deformations to Einstein gravity and find the exact configurations for the complete theory, discussing all the different branches exhaustively. One of the effects of introducing the Chern-Simons gravitational term is that of breaking the degeneracy in the effective mass of the generic modes of pure New Massive Gravity, producing a fine structure due to parity violation. Another effect is that the zoo of exact logarithmic specimens becomes considerably enlarged.