Homogeneous Solutions of Minimal Massive 3D Gravity
arXiv:1703.06871 · doi:10.1103/PhysRevD.96.026024
Abstract
In this paper we systematically construct simply transitive homogeneous spacetime solutions of the three-dimensional Minimal Massive Gravity (MMG) model. In addition to those that have analogs in Topologically Massive Gravity, such as warped AdS and pp-waves, there are several solutions genuine to MMG. Among them, there is a stationary Lifshitz metric with the dynamical exponent z=-1 and an anisotropic Lifshitz solution where all coordinates scale differently. Moreover, we identify a homogeneous Kundt type solution at the chiral point of the theory. We also show that in a particular limit of the physical parameters in which the Cotton tensor drops out from the MMG field equation, homogeneous solutions exist only at the merger point in the parameter space if they are not conformally flat.
23 pages, v2: minor changes, references added
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Cited by in corpus (7)
- Spontaneously Broken 3d Hietarinta/Maxwell Chern-Simons Theory and Minimal Massive Gravity
- Supersymmetric Solutions of N = (1,1) General Massive Supergravity
- Thermodynamic Stability of the Stationary Lifshitz Black Hole of New Massive Gravity
- Circularly symmetric solutions of Minimal Massive Gravity at its merger point
- Matter coupling in Minimal Massive 3D Gravity and spinor-matter interactions in exterior algebra formalism
- Brief Note on Thurston Geometries in 3D Quadratic Curvature Theories
- A note on the pp-wave solution of Minimal Massive 3D Gravity coupled with Maxwell-Chern-Simons theory