Matter coupling in 3D "Minimal Massive Gravity"
arXiv:1407.1264 · doi:10.1088/0264-9381/31/23/235012
Abstract
The "Minimal Massive Gravity" (MMG) model of massive gravity in three spacetime dimensions (which has the same anti-de Sitter (AdS) bulk properties as "Topologically Massive Gravity" but improved boundary properties) is coupled to matter. Consistency requires a particular matter source tensor, which is quadratic in the stress tensor. The consequences are explored for an ideal fluid in the context of asymptotically de-Sitter (dS) cosmological solutions, which bounce smoothly from contraction to expansion. Various vacuum solutions are also found, including warped-(A)dS, and (for special values of parameters) static black holes and an (A)dS2 x S1 vacuum.
19 pages. v2 includes simplifications due to an improved parametrisation, and an explicit verification of the main result. Minor corrections made and additional references added in v3
References in corpus (6)
Cited by in corpus (7)
- Minimal Massive Gravity: Conserved Charges, Excitations and the Chiral Gravity Limit
- Black hole conserved charges in Generalized Minimal Massive Gravity
- Minimal Massive 3D Gravity Unitarity Redux
- Yang-Mills as massive Chern-Simons theory: a third way to three-dimensional gauge theories
- On Solutions of Minimal Massive 3D Gravity
- The entropy formula of black holes in Minimal Massive Gravity and its application for BTZ black holes
- Bulk and Boundary Unitary Gravity in 3D: MMG